The galaxy presents as an elliptical or lenticular morphology. The central bulge exhibits a smooth, concentrated light profile, indicating a high stellar density, likely dominated by older stellar populations. The overall color appears to be yellowish to reddish, suggestive of a low star formation rate and a population dominated by evolved stars. There is a slight elongation in the shape, which could be indicative of a mild tidal disturbance or interaction with a smaller galaxy, which is possibly seen to the bottom-left of the larger galaxy. The overall structure appears relatively undisturbed, with no prominent spiral arms or dust lanes visible.
