The galaxy presents a generally smooth, elliptical morphology with a slight elongation. Its central region exhibits a high degree of luminosity, indicating a concentration of stars or active galactic nucleus activity. The light profile transitions gradually from the core to the outer regions, which appear fainter and more diffuse. There is a subtle color gradient, with the central region appearing more yellow and the outer regions exhibiting a slightly redder hue. The galaxy appears relatively undisturbed, with no prominent signs of recent major mergers or tidal interactions, though a slight asymmetry in the outer regions cannot be ruled out. No distinct spiral arm structures or prominent dust lanes are discernible. Overall, the galaxy appears to be a relatively mature system, consistent with an early-type classification.
