The galaxy presents as a centrally concentrated, relatively smooth elliptical galaxy. Its overall shape is largely spheroidal. The color profile indicates a prominent, luminous core that transitions to a more diffuse, reddish halo. No distinct spiral arm structures or dust lanes are discernible. There is no evidence of any major mergers or tidal disturbances, indicating that it is likely an undisturbed, mature system. It seems to be composed primarily of older stellar populations.
