The galaxy presents as a centrally concentrated, elliptical-like system with a smooth overall light distribution. It exhibits a noticeable central bulge that appears bright and slightly off-white in color. Extending outward from the core is a fainter, more diffuse halo. There is a subtle suggestion of an extended disk-like component, though the lack of distinct spiral arm structures suggests it is likely a lenticular or early-type spiral. The galaxy's color is slightly blue, indicative of some ongoing star formation. The galaxy's shape is slightly flattened, appearing more 'in-between' than perfectly round or cigar-shaped. Overall, there appears to be no significant indication of major mergers or tidal disruptions, though there may be some minor disturbance of the surrounding stars.
