The galaxy appears as an elliptical-like structure, with a bright, concentrated central bulge dominating the overall luminosity. The light distribution appears relatively smooth, suggesting an older stellar population. The galaxy has a moderate apparent size. It has a slight disk-like shape. There are no prominent dust lanes or spiral arm structures visible. The overall color is a pale blue to white, indicative of a mixed stellar population. The edges of the galaxy fade gradually into the background, and the light is concentrated towards the center. There are no signs of major interaction or merging events, such as tidal tails or distorted morphology, though there are minor disturbances.
