The galaxy presents a generally smooth and concentrated morphology, indicative of a spheroid-dominated system. Its apparent shape is approximately elliptical, though close to circular, with no discernible spiral arms or distinct features like a prominent bar or ring structures. The light profile appears to be centrally concentrated with a gradual decrease in intensity outwards from the nucleus, suggesting a relatively old stellar population. There is a distinct color gradient visible, with the central region exhibiting a yellowish hue that transitions to slightly redder colors in the outer regions. There is no evidence of ongoing major mergers or tidal disturbances, although some minor asymmetries might be present in the outer isophotes which could suggest a past interaction or accretion event. Overall the galaxy appears to be a relatively quiescent system, with a smooth light distribution indicative of an early-type galaxy undergoing little current star formation.
