NGC 4408 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Virgo. It is part of the Virgo Cluster, a group of galaxies that includes many other notable members. NGC 4408 has a diameter of about 70,000 light-years and is characterized by its bright central bar structure and spiral arms. Discovered by the astronomer William Herschel in 1784, NGC 4408 is notable for its relatively high surface brightness, making it easier to observe with telescopes. The galaxy exhibits signs of interaction with nearby galaxies, which can influence its shape and star formation activities.