The galaxy appears to be undergoing a significant interaction, potentially a merger. The primary body presents a somewhat elliptical morphology, but is severely disturbed. There is an indication of tidal tails or other debris extending away from the main body. One region of the galaxy is more luminous and centrally located, with what appears to be a high concentration of older stars. Another part of the galaxy appears to be more diffuse, with a bluer color indicating younger stars. The overall appearance suggests a complex gravitational interaction has taken place, significantly impacting the morphology and star formation activity within this galaxy. A possible dust lane is present.
