The galaxy presents as a relatively smooth, elliptical morphology, exhibiting a concentrated central bulge. There is a noticeable color gradient, with the central region displaying a yellowish hue, potentially indicative of an older stellar population. The outer regions appear slightly bluer, suggesting the presence of some younger stars, but these do not form distinct spiral arm structures. The galaxy's overall shape is somewhere between round and elongated. No major disturbances or signs of ongoing mergers are readily apparent, although there is possibly a hint of a minor irregularity along one edge.
