The galaxy presents a generally smooth and elliptical morphology. The light is centrally concentrated, with a gradual decrease in brightness towards the edges. There is little evidence of spiral arms or significant dust lanes. The overall color appears to be moderately red-shifted, suggesting a population of older stars. There is a slight asymmetry with a subtle extension of the isophotes in one direction. The galaxy appears relatively undisturbed, with no clear signs of ongoing major mergers or tidal interactions. 
