Galaxy Morphology

Galaxy morphology refers to the classification and appearance of galaxies based on their shape and structure. Generally, galaxies are categorized as spiral (with rotating disks, arms, and central bulges), elliptical (more rounded and featureless), or irregular (lacking distinct shape). These shapes result from their formation processes, interactions, and evolutionary history. Studying galaxy morphology helps astronomers understand how galaxies form, evolve, and interact within the universe. It provides a way to organize and compare galaxies, revealing insights into their life cycles and the dynamics of the cosmos.