This galaxy exhibits a complex morphology, potentially indicating an ongoing or past interaction with another galaxy. The primary body of the galaxy appears relatively smooth and elliptical in shape, suggesting a significant population of older stars. However, a distinct, brighter, and more concentrated region is evident, possibly representing a galactic nucleus or a region of enhanced star formation. This secondary concentration displays a slightly different color profile, appearing more yellow-orange, which could indicate a higher abundance of dust or a younger stellar population compared to the overall galaxy. A faint bridge of material seems to connect the primary body with the secondary concentration. There are possible signs of tidal disturbances around the edges of the galaxy, such as faint streams or extended halos. These features support the interpretation of this galaxy being in a state of transition or merger. Overall, the galaxy appears to be a massive system with a significant star formation rate.
