The galaxy exhibits a flattened, elliptical morphology. It appears relatively smooth in structure with no obvious spiral arms or bar. The central region is bright and concentrated, suggesting a prominent bulge. The overall color is slightly yellowish, indicating an older stellar population. The galaxy shows some hints of a disk structure extending from the central bulge. There is some marginal evidence of a minor disturbance, likely an interaction or past merger. There are no pronounced tidal tails or other merger remnants directly apparent in the image.
