Irregular galaxies are defined by several key characteristics:
Irregular galaxies are further classified into two subtypes:
The irregular shape of these galaxies is often attributed to disruptive gravitational interactions with other galaxies. They may have been formed as a result of galactic collisions or gravitational disturbances, leading to their irregular appearance.
Irregular galaxies can be observed using telescopes equipped with high-resolution imaging capabilities. Observing the distribution of stars, gas, and dust within these galaxies can provide valuable insights into their formation and evolution.
When studying irregular galaxies, it's important to focus on the following key points: