As part of the FIRE project, we have simulated a large number of galaxies that resemble the Milky Way or Andromeda, including some "Local Group" systems which include both, together, like our own neighborhood. Shea Garrison-Kimmel has compiled a large number of movies of these different systems, side-by-side, such as the example shown below. His page (with a huge number of different movies showing the gas and stars in all these systems or each of them at a time) allows you to see the diversity of formation and merger histories, that produce galaxies broadly similar to our own today.
The movies below are constructed from these and other simulations which show a variety of behaviors, from dwarf galaxies that form thick, puffy gas disks to Milky Way or Local Group-type systems. In all cases, the starlight images are mock u/g/r composite Hubble Space Telescope-type images (blue shows sites of young star formation, red/brown shows where dust has obscured the starlight). The gas images are a mock three-color composite showing the cold neutral gas (magenta, < 8000 K), warm ionized gas (green, ~1e4 - 1e5 K), and hot gas (red, >1e6 K). For each galaxy, there are two or four videos, showing gas and stars, and (if four) one "zoomed in" on small scales, with another "zoomed out" on large scales.
These simulations were primarily run by Andrew Wetzel and Shea Garrison-Kimmel (m11b by TK Chan), and are discussed in https://arxiv.org/abs/1806.04143. Images of the galaxies at the present day can be found here. Credit for making the movies goes to Shea Garrison-Kimmel (variants of these movies that go faster or slower, or have higher resolution, or tile the movies together, are available upon request from Shea).

m11b: Disky Dwarf (Gas)

m11b: Disky Dwarf (Stars)

A Local Group: the large-scale view (Gas, 1500kpc)

A Local Group: the large-scale view (Stars, 1500kpc)

Romeo: Andromeda-like with an extended disk (Gas, 40kpc)

Romeo: Andromeda-like with an extended disk (Stars, 40kpc)

Romeo: Andromeda-like with an extended disk (Gas, 400kpc)

Romeo: Andromeda-like with an extended disk (Stars, 400kpc)

Juliet: Milky Way-like with vigorous star formation (Gas, 40kpc)

Juliet: Milky Way-like with vigorous star formation (Stars, 40kpc)

Juliet: Milky Way-like with vigorous star formation (Gas, 400kpc)

Juliet: Milky Way-like with vigorous star formation (Stars, 400kpc)

m12b: Milky Way-mass, with a more compact disk (Gas, 40kpc)

m12b: Milky Way-mass, with a more compact disk (Stars, 40kpc)

m12b: Milky Way-mass, with a more compact disk (Gas, 400kpc)

m12b: Milky Way-mass, with a more compact disk (Stars, 400kpc)

m12c: An older, redder disk galaxy (Gas, 40kpc)

m12c: An older, redder disk galaxy (Stars, 40kpc)

m12c: An older, redder disk galaxy (Gas, 400kpc)

m12c: An older, redder disk galaxy (Stars, 400kpc)

m12f: If the Milky Way ate the LMC… (Gas, 40kpc)

m12f: If the Milky Way ate the LMC… (Stars, 40kpc)

m12f: If the Milky Way ate the LMC… (Gas, 400kpc)

m12f: If the Milky Way ate the LMC… (Stars, 400kpc)

m12i: Milky Way-like but with a thicker, younger disk (Gas, 40kpc)

m12i: Milky Way-like but with a thicker, younger disk (Stars, 40kpc)

m12i: Milky Way-like but with a thicker, younger disk (Gas, 400kpc)

m12i: Milky Way-like but with a thicker, younger disk (Stars, 400kpc)

m12m: An extended, barred disk (Gas, 40kpc)

m12m: An extended, barred disk (Stars, 40kpc)

m12m: An extended, barred disk (Gas, 400kpc)

m12m: An extended, barred disk (Stars, 400kpc)

m12r: A late major merger destroys the disk (Gas, 40kpc)

m12r: A late major merger destroys the disk (Stars, 40kpc)

m12r: A late major merger destroys the disk (Gas, 400kpc)

m12r: A late major merger destroys the disk (Stars, 400kpc)

m12w: An early-forming, bulge-dominated S0 (Gas, 40kpc)

m12w: An early-forming, bulge-dominated S0 (Stars, 40kpc)

m12w: An early-forming, bulge-dominated S0 (Gas, 400kpc)

m12w: An early-forming, bulge-dominated S0 (Stars, 400kpc)

m12z: A lower-mass, low surface-brightness disk (Gas, 40kpc)

m12z: A lower-mass, low surface-brightness disk (Stars, 40kpc)

m12z: A lower-mass, low surface-brightness disk (Gas, 400kpc)

m12z: A lower-mass, low surface-brightness disk (Stars, 400kpc)