The galaxy presents as a roughly elliptical morphology with a smooth light distribution, suggesting a relatively old stellar population. There is a slight elongation evident in the major axis. The central region exhibits a concentrated, brighter luminosity profile compared to the outer regions, which appear fainter and more diffuse. Some faint blue color is subtly detected in the outskirts. There is no strong evidence of spiral arms, dust lanes, or active star-forming regions from this image. The galaxy appears relatively undisturbed. The color profile hints at a redder core transitioning to a slightly bluer halo.
