The galaxy presents an elliptical morphology, appearing somewhat smooth in texture, yet shows signs of substructure that may indicate a disk. The central bulge is bright and concentrated, suggesting a high density of stars. Moving outward from the core, the galaxy appears less concentrated. The overall color profile suggests the presence of older stellar populations. A slight asymmetry is present, but the galaxy does not obviously exhibit signs of a major merger event or significant tidal disturbances. There is a possible minor disturbance or interaction on the periphery, though it is difficult to discern. Overall, the galaxy appears relatively undisturbed.
