The galaxy presents a largely smooth and elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness extending outwards. The galaxy appears to be more elongated than circular, but not extremely so. A slight colour gradient is present, with a hint of a bluer hue in the outer regions compared to the central bulge, which exhibits a more yellow colour. Overall, the galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions.
