The galaxy presents as a relatively smooth and centrally concentrated object, exhibiting an overall elliptical morphology. The core region appears bright and somewhat diffuse, suggesting a high stellar density and potentially an active galactic nucleus or recent star formation. The light profile transitions gradually from the central bulge to the outer regions, indicating a lack of distinct spiral arm structure.

There is a slight elongation to the galaxy's shape, more closely categorized as "in between" round or cigar shaped. This implies a potential deviation from perfect sphericity. Faint color variations are observable throughout the galaxy, with a somewhat redder hue near the center, transitioning toward a more bluer color in the outskirts. No major disturbances, strong tidal features, or ongoing mergers are readily apparent, though there could be a minor disturbance in the galaxy.
