The galaxy presents a flattened, elliptical morphology. Its core exhibits a bright, concentrated luminosity gradient, suggesting a high stellar density within the central region. The surrounding halo displays a more diffuse and less luminous distribution of stars. A subtle bluing effect is observed in the outer regions, possibly indicating the presence of a younger stellar population compared to the predominantly yellow core. The overall structure appears relatively undisturbed, showing no obvious signs of tidal interactions or ongoing major mergers. There are some hints of disturbances in the morphology, but they are minor. The galaxy has an intermediate apparent roundness.
