NGC 4407 is a barred spiral galaxy located in the constellation Virgo. It is approximately 60 million light-years away from Earth and is part of the Virgo Cluster, a group of galaxies that are gravitationally bound together. This galaxy has a diameter of about 70,000 light-years and is classified as type SBc, indicating its spiral structure with a central bar. NGC 4407 is notable for its bright core and the presence of star-forming regions, which contribute to its overall luminosity and visual appeal in astronomical observations.