The galaxy presents a largely smooth and rounded morphology. It exhibits a bright, concentrated core that transitions into a more diffuse halo. The galaxy has a somewhat elliptical shape, with a slight deviation from perfect circularity. The color profile suggests a dominant population of older stars, with a redder hue concentrated towards the center and a gradual shift to slightly bluer tones in the outer regions. There is no evidence of a prominent disk structure, spiral arms, or significant dust lanes. The galaxy appears relatively undisturbed, showing no obvious signs of recent mergers or tidal interactions.
