NGC 3396
NGC 3396 is a barred spiral galaxy located in the constellation Leo. It is approximately 50 million light-years away from Earth and is part of the Virgo Cluster, which contains many other galaxies. NGC 3396 is notable for its bright core and well-defined spiral arms, making it an interesting subject for astronomers.
Discovered by William Herschel in 1784, NGC 3396 has a diameter of about 70,000 light-years. Its structure and composition provide valuable insights into the formation and evolution of galaxies. Observations of NGC 3396 contribute to our understanding of cosmic phenomena and the dynamics of galactic interactions.