This galaxy exhibits an elliptical morphology. The central region is dominated by a bright, concentrated bulge, indicating a significant population of older stars. Extending outward from the core, the galaxy shows a smooth, diffuse halo. The overall shape is elongated, with a high degree of ellipticity, and the disk appears relatively faint in comparison to the bulge. The galaxy's color suggests that star formation is relatively low. There is also a slight disturbance on the left side of the galaxy, perhaps indicative of a minor interaction with a small galaxy.