The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, centrally bright bulge with a gradual decrease in surface brightness towards the edges. There is very little, if any, evidence of spiral arm structure or significant dust lanes. The galaxy's shape is somewhat elongated, suggesting a possible deviation from a perfectly spherical morphology. The color is generally yellow/orange, indicating a stellar population dominated by older, redder stars with a low rate of ongoing star formation. There is also a slight chance this galaxy could be in the process of merging or has undergone a minor disturbance, as it appears asymmetric, but this is not clearly evident.
