The galaxy appears to be an elliptical galaxy. Its morphology is generally smooth and rounded in shape. There is a very bright central bulge that appears roughly circular. The concentration of light is highest at the center, gradually decreasing towards the outer regions. Faint extensions can be seen surrounding the central body, suggesting the presence of a stellar halo. There is no evidence of spiral arms or significant dust lanes, indicating that the galaxy is an early-type galaxy. There does not appear to be any evidence of any current ongoing merging events, and the galaxy does not appear to be highly disturbed.
