NGC 125 is a spiral galaxy located in the constellation of Cetus. It is approximately 70 million light-years away from Earth and is part of the Peculiar Galaxy group. NGC 125 is notable for its distinct spiral structure and bright central region, which contains a high concentration of stars. Discovered in 1886 by astronomer Édouard Stephan, NGC 125 has been the subject of various astronomical studies. Its features make it an interesting object for both amateur and professional astronomers, contributing to our understanding of galaxy formation and evolution in the universe.