NGC 4414 is a spiral galaxy located approximately 60 million light-years away in the constellation Coma Berenices. It is classified as a type Sc spiral galaxy, characterized by its loosely wound arms and a bright central bulge. This galaxy spans about 50,000 light-years in diameter and is notable for its lack of significant dust lanes, which is unusual for spiral galaxies. NGC 4414 is part of the Virgo Supercluster and is often studied to understand galaxy formation and evolution.