The Milky Way is classified as a barred spiral galaxy, characterized by its prominent spiral arms extending from a central bar-shaped structure.

Elliptical galaxies are distinguished by their smooth, round or elliptical appearance, lacking prominent spiral arms or irregular structures.

Irregular galaxies are characterized by their lack of a well-defined shape, exhibiting chaotic and fragmented structures.

Lenticular galaxies, also known as S0 galaxies, possess a central bulge similar to elliptical galaxies but also have a flattened disk structure.

Sagittarius A* is the supermassive black hole located at the center of our Milky Way galaxy, with a mass estimated to be millions of times that of our Sun.

Andromeda, also known as M31, is the closest major galaxy to our Milky Way, located approximately 2.5 million light-years away.

Galactic mergers occur when two or more galaxies collide and combine to form a single, larger galaxy.

Starburst galaxies are characterized by an intense burst of star formation, resulting in a high concentration of young, massive stars.

Active galactic nuclei (AGNs) are the extremely luminous centers of galaxies powered by the accretion of matter onto a supermassive black hole.

Seyfert galaxies are a type of active galaxy characterized by their bright, narrow emission lines, indicating the presence of ionized gas near the supermassive black hole.

Quasars are extremely luminous active galaxies that emit vast amounts of energy, often outshining entire galaxies, and are powered by supermassive black holes.

Spiral galaxies, like our Milky Way, consist of a central disk containing stars, gas, and dust, surrounded by a halo of stars, gas, and dark matter.

Andromeda, also known as M31, is a large, barred spiral galaxy located approximately 25 million light-years away from Earth and is the closest major galaxy to our Milky Way.

Lenticular galaxies, also known as S0 galaxies, have a central bulge and a surrounding disk, but lack the prominent spiral arms characteristic of spiral galaxies.

Galactic evolution refers to the processes by which galaxies change and develop over time, including the formation of stars, the merging of galaxies, and the interactions between galaxies and their environments.