Galaxies form through the gravitational collapse of gas clouds and the subsequent condensation of matter into stars and stellar systems. The precise mechanisms driving galaxy formation are complex and multifaceted, involving processes such as hierarchical merging, accretion of gas, and feedback from star formation and active galactic nuclei. Over billions of years, these processes give rise to the diverse array of galaxies observed in the universe today.
Come for the Scenery, Stay for the Stars