The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge of yellowish-white light, indicative of an older stellar population. The galaxy appears to be largely featureless, lacking prominent spiral arms or dust lanes. The outer regions of the galaxy display a subtle, diffuse halo extending beyond the core, suggesting a gradual decrease in stellar density. The overall shape appears elongated, but not excessively so, trending towards a cigar-like appearance, with the major axis displaying a significant, although not extreme, angular size. There is a minor hint of a possible faint tidal feature or disturbance on one side, but further analysis would be required to confirm if this is a genuine interaction. The color gradient from the core to the outer regions is subtle, but the outer regions exhibit slightly bluer tones, which could indicate some ongoing, albeit low-level, star formation activity.
