NGC 2015 is a bright nebula located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is part of a larger region known as the LMC and is situated approximately 163,000 light-years from Earth. This nebula is notable for its vibrant colors and intricate structure, which are the result of intense star formation. The nebula is often studied by astronomers to understand the processes of star birth and the dynamics of interstellar gas and dust. NGC 2015 contains several young, hot stars that emit strong ultraviolet radiation, contributing to the ionization of surrounding gas and creating its characteristic glow.