The galaxy presents as a smooth, elliptical-like structure. There appears to be a brighter central region, possibly indicative of a galactic nucleus or a concentration of older stars. The light distribution suggests a bulge-dominated morphology, with a gradual decrease in intensity outward from the center, though with some fuzziness. Its overall shape is elongated, with a hint of a cigar-like form, indicating that it is not perfectly spherical. There are faint, diffuse halos or tidal features in the outer regions, suggestive of past minor interactions or internal dynamical processes. There's a possible disturbance of the main structure. The galaxy exhibits a color gradient, with a bluer hue concentrated in the center and a redder hue in the outer regions, consistent with the presence of both young and old stellar populations.
