NGC 4779
NGC 4779 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Virgo. It was discovered by the astronomer William Herschel in 1784. The galaxy is notable for its bright core and well-defined spiral arms, which are characteristic features of spiral galaxies.
This galaxy is part of the Virgo Cluster, a group of galaxies that includes many other notable members. NGC 4779 has been studied for its star formation activity and the presence of various stellar populations, providing insights into the evolution of galaxies in the universe.