The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical or lenticular type. The overall shape is somewhat elongated, appearing as "in between" round and cigar-shaped. A central, bright region indicates a possible concentration of stars or potentially an active galactic nucleus, though the resolution does not allow for definitive determination. Subtle color gradients are observed, transitioning from a bluer hue in the outer regions to a slightly redder tone towards the core. There is no strong evidence of spiral arms or significant dust lanes. The galaxy does not appear to be undergoing a major merger, although the possibility of a minor disturbance or past interaction cannot be entirely ruled out. Overall, the galaxy seems to be relatively quiescent, with no apparent signs of intense star formation activity.
