The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of radial symmetry. The light distribution appears concentrated towards the center, suggesting a significant bulge component. Color gradients are subtle but noticeable. The core region displays a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions are slightly bluer, hinting at the presence of younger stars, though the overall star formation activity appears to be relatively low. There may be some minor disturbances from mergers and tidal events, but none are immediately obvious. The galaxy appears quite round, showing no strong elongation or disk-like features. 
