The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central region, with a gradual decrease in luminosity towards its outer edges. The central region appears yellowish, suggesting a population of older stars. Fainter, diffuse regions are observed around the central bulge, with a slight elongation that isn't quite cigar shaped. There is no obvious sign of spiral arm structure or major disturbances in the image. No prominent tidal tails or merging features are detected, though some small irregularity exists within the faint, outer halo.
