NGC 414 is a spiral galaxy located in the constellation of Pisces. It is approximately 70 million light-years away from Earth and is part of the Pisces-Perseus Supercluster. NGC 414 is notable for its distinct spiral structure, which is characterized by well-defined arms that contain young stars and regions of active star formation. Discovered by the astronomer John Herschel in 1831, NGC 414 is classified as a type Sc spiral galaxy. Its brightness and structure make it an interesting object for both amateur and professional astronomers. Observations of NGC 414 contribute to our understanding of galaxy formation and evolution in the universe.