Unbalanced galaxies, often referred to as irregular galaxies, lack a distinct shape or structure. Unlike spiral or elliptical galaxies, they do not have a well-defined form, which can result from gravitational interactions with other galaxies or internal processes. These galaxies can contain a mix of young and old stars, gas, and dust, contributing to their chaotic appearance. The irregular shape of unbalanced galaxies can also lead to active star formation, as regions of gas and dust collapse under gravity. Examples of unbalanced galaxies include the Large Magellanic Cloud and the Small Magellanic Cloud, both of which are satellite galaxies of the Milky Way.