The galaxy presents as a largely featureless, elliptical morphology with a high degree of central concentration. The light profile appears smooth and regular, suggestive of an evolved stellar population. The color gradient transitions from a bright, yellowish core to a redder outer halo, potentially indicative of older stars dominating the outskirts and younger stars dominating the core. There is no discernible spiral structure or dust lanes visible within the galaxy's isophotes. Its apparent roundness suggests a nearly face-on orientation with no significant merging activity disrupting the overall structure. The lack of distinct features would indicate that it is a quiescent galaxy with minimal recent star formation.
