The galaxy presents a generally smooth and elliptical morphology. There is a bright, concentrated central bulge that appears nearly spherical. The surrounding halo exhibits a gradual decrease in luminosity extending outwards with a slight elongation. The color profile suggests a population of older stars, especially toward the core, with a subtle bluer hue in the outer regions, possibly indicating ongoing star formation. The galaxy appears relatively undisturbed, without any obvious signs of recent major mergers or tidal interactions.
