The galaxy presents as a relatively smooth, elliptical-like structure. The central region displays a concentrated, bright core, transitioning outwards to a more diffuse halo. Coloration suggests a population of older stars, with a redder hue dominating the overall appearance. There is a subtle color gradient from the center to the edge, suggesting a possible radial change in stellar populations or dust content. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or tidal interactions.
