NGC 4577
NGC 4577 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Virgo. It is part of the Virgo Cluster, which contains thousands of galaxies. NGC 4577 has a bright central region and well-defined spiral arms, making it an interesting object for astronomers.
This galaxy is notable for its active nucleus, which is believed to host a supermassive black hole. Observations of NGC 4577 contribute to our understanding of galaxy formation and evolution, particularly in relation to the interactions between galaxies within clusters like Virgo.