The galaxy presents a generally smooth, rounded morphology, indicative of an elliptical galaxy type, but with the suggestion of a weak disk-like structure. The central region exhibits a high surface brightness, concentrated in a near spherical core that gradually diffuses outwards. Some asymmetry can be observed in the outer regions, potentially indicative of a past interaction or minor disturbance. The color profile indicates a relatively homogenous stellar population. Overall, the galaxy's appearance suggests a dynamically relaxed system, yet the subtle features imply an ongoing or recent interaction.