The galaxy presents as a largely featureless elliptical object. It exhibits a smooth, centrally concentrated light profile, with a gradual decrease in luminosity extending outwards from the core. The core region appears bright and yellowish, suggesting a population of older stars. The overall shape is close to elliptical with a round appearance, with no apparent spiral arms or prominent disk-like structures are discernable. There is only the slightest hint of a disk. No major signs of ongoing merger activity are visible. A very slight disturbance may be seen in the left of the galaxy, although it is not certain. Based on the color and lack of structure, this galaxy is likely a mature system with relatively low star formation rate.
