The galaxy presents as a smooth, elliptical morphology. The light is concentrated towards the center, indicating a substantial bulge. The isophotes appear generally smooth, with no obvious strong features such as spiral arms or a bar. The color gradient suggests a population of older stars, particularly within the central region, potentially with some dust. The elongation may indicate a weak disk component or a triaxial structure. No signs of major mergers or tidal disturbances are apparent.
