Spiral Galaxies
Characterized by their spiral arms that extend from a central bulge, spiral galaxies are home to active star formation. Our own Milky Way is a prime example.
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Elliptical Galaxies
These galaxies are smooth, featureless, and range from nearly spherical to highly elongated. They typically contain older stars and have little gas or dust.
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Irregular Galaxies
Lacking a distinct regular shape, these galaxies often result from gravitational disturbances or collisions. They can be rich in gas and dust, fostering new stars.
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Lenticular Galaxies
Positioned between spirals and ellipticals, lenticular galaxies have a central bulge and a disk but lack significant spiral arms. They contain mostly older stars.
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