The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density or possible active galactic nucleus. The light from the central region appears yellow, shifting toward redder tones in the outer regions, indicating an older stellar population. There's a noticeable lack of defined spiral arms or prominent dust lanes, which is consistent with elliptical galaxy morphology. The overall shape is closer to an oval but not elongated to the point of being cigar-shaped. There is no indication of strong tidal disturbances, major mergers, or significant asymmetry.
