The galaxy presents as a moderately luminous, elliptical or lenticular system. Its morphology is primarily smooth and exhibits a high degree of central concentration. The light profile is generally smooth and symmetrical, with a shallow gradient towards the outer edges. A subtle reddish hue dominates the central region, suggesting a population of older stars, while a slight greenish tint in the surrounding area could indicate the presence of some younger stars or ongoing, but subdued, star formation. There is no apparent dust lane or prominent spiral arm structure. The galaxy appears relatively undisturbed, showing no obvious signs of tidal interactions or recent major mergers.
