The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing nearly spheroidal and dominating the galaxy's overall luminosity. This suggests a significant concentration of older stellar populations in the core. The outer regions gradually fade in intensity, displaying a more diffuse halo with a slightly elongated form; there is a very slight disc appearance when looking from the center out toward the edge of the galaxy, though it has mostly been absorbed by the overall spheroidal shape. A subtle tidal tail may be present on one side, potentially indicating a minor past interaction, though this feature is not a major disturbance. Overall, the galaxy appears relatively isolated and undisturbed.
