The galaxy presents an elliptical morphology, though some disk features may be present. It appears to be generally smooth in structure, but some evidence of minor disturbances cannot be ruled out. The galaxy's shape is somewhat elongated with an estimated axial ratio of approximately 0.64. The color gradient suggests a relatively passive stellar population towards the center, indicated by the yellowish core, with bluer colors extending outwards within the galaxy's body. The galaxy exhibits a relatively high Sersic index, indicating a centrally concentrated light profile. Despite the apparent smoothness, faint hints of asymmetrical features can be observed, implying possible past or ongoing interactions or mergers.
