The galaxy presents as a single, concentrated object, exhibiting a smooth and primarily spheroidal morphology. Its color profile suggests an older stellar population, with a yellow/orange hue dominating the central region. There is little evidence of distinct spiral arms or significant dust lanes; instead, the light is distributed relatively evenly across the galaxy. Some minor asymmetrical disturbances are present. The overall structure appears relatively undisturbed with some possible signs of tidal features, potentially indicating an ongoing or past interaction with a smaller companion galaxy. The galaxy's light profile decreases gradually from the center outwards.