The galaxy presents as a centralized, smooth elliptical or lenticular structure, displaying a gradual decline in surface brightness from core to edge. Its overall shape is somewhat elongated, but not highly so. It appears mostly undisturbed with no prominent tidal features or signs of ongoing major mergers. There may be some minor irregularities or substructure present, possibly indicating minor disturbances. The galaxy appears to have a low ongoing star formation rate.
