The galaxy appears as a relatively smooth, elliptical or lenticular object. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. There is a subtle color gradient, with the central regions exhibiting a slightly yellower or redder hue compared to the outer regions which appear bluer, suggesting a mixed stellar population. Faint indications suggest that the galaxy may possess a weak, unresolved disk component. The overall shape is close to round. No significant signs of tidal disturbances or major merging events are apparent, but there are possibly minor disturbances present, indicative of a potential past interaction or ongoing accretion. The galaxy is of moderate size. The rate of star formation seems mild.
