The galaxy presents as an elliptical or lenticular morphology, exhibiting a flattened, disk-like structure. A bright, concentrated bulge is visible at the galaxy's center, suggesting a significant population of older stars. The overall color of the galaxy is yellowish-white, indicating a relatively low rate of ongoing star formation. Some slight irregularities are present, indicating the possibility of a minor disturbance to the galaxy. There is no definitive evidence of major mergers. The halo exhibits a smooth light distribution.
