The galaxy presents a generally smooth and elliptical morphology. A bright central bulge is apparent, with a gradual decrease in luminosity extending outwards. Faint, disk-like features are tentatively observed, suggesting a possible spiral structure viewed at a high inclination, but these are subtle. The color profile indicates a possible gradient from redder hues in the bulge to slightly bluer tones in the outer regions of the disk, which may be indicative of differing stellar populations, with older stars dominating the core and a possible, small amount of ongoing star formation within the faint, disk-like structure. No strong signs of tidal disturbances or ongoing mergers are immediately apparent.
