The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards. The overall color is yellowish-orange, suggestive of an older stellar population and lower rates of current star formation. There is no significant evidence of spiral arms or prominent dust lanes. The shape is mostly rounded, with no indication of major disturbances from mergers or tidal interactions. There might be a slight asymmetry, but this is not clearly defined. The size appears compact, with light concentrated towards the center.
