An irregular galaxy is a type of galaxy that does not have a distinct regular shape, unlike spiral or elliptical galaxies. These galaxies are often chaotic in appearance, with no defined structure or symmetry. Irregular galaxies can be further classified into two subtypes: Irr I and Irr II.
Irr I galaxies are characterized by their relatively high levels of dust and gas, as well as ongoing star formation. They often exhibit a more organized structure compared to Irr II galaxies, with some regions showing hints of spiral arms or other features.
Irr II galaxies, on the other hand, are more chaotic in nature, lacking any distinct structure or symmetry. They typically have lower levels of dust and gas, with little ongoing star formation. These galaxies are often the result of gravitational interactions with other galaxies, leading to their irregular appearance.