The galaxy presents as an elliptical or lenticular structure, exhibiting a smooth, centrally concentrated light profile. The core region is notably bright and diffuse, suggesting a high stellar density. Progressing outwards, the light gradually fades into a more extended halo or disk component. The galaxy's overall shape appears elongated, deviating from a perfect sphere. There are hints of asymmetry in the outer regions, although no major disturbances or tidal features are immediately apparent in this view. The color indices suggest a population of older stars, with a reddish-yellow hue dominating the galaxy's overall appearance. Subtle color gradients are visible, possibly indicating variations in stellar populations or dust content across the galaxy's structure.
