The galaxy presents a smooth, elliptical morphology. The central region exhibits a concentrated, bright core, transitioning outward to a more diffuse halo. The color profile suggests a dominant population of older stars, with a yellowish-red hue in the core region. The outer regions display a slightly bluer tint, possibly indicating some younger stellar populations or ongoing star formation, though the overall color suggests this is minimal. No distinct spiral arms or features are discernible. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent mergers. Its shape is somewhat elongated but generally rounded rather than cigar-shaped. Minor structural irregularities or disturbances appear to be present, but these are not significant.
