The galaxy appears as a smooth, elliptical-shaped structure. It exhibits a concentrated central bulge that dominates the light distribution. The color profile suggests a relatively old stellar population with a yellow-red hue, with the central bulge appearing the most intensely colored. There is a subtle color gradient from the center outwards. There is no strong evidence of spiral arm structures or significant dust lanes. The galaxy appears relatively undisturbed, lacking obvious signs of recent major mergers or tidal interactions.
