The galaxy presents a generally smooth, elliptical morphology. A dominant central bulge is observed, appearing bright and concentrated. The light from this central region is predominantly yellow, suggesting an older stellar population. The outer regions of the galaxy exhibit a fainter and more diffuse halo. There is a suggestion of disk-like features, though these are not prominent. Faint tidal disturbances are visible in the halo, indicating a possible past interaction or merger event. Star formation is low, which is expected based on the older stellar population present. The shape appears close to round and the object appears mostly undisturbed.
