The galaxy presents as a centrally concentrated, elliptical-like structure. The light profile appears smooth and diffuse, with a noticeable lack of distinct spiral arms or prominent dust lanes. The core region exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. Moving outward from the center, the color gradually shifts towards a slightly bluer tint, potentially indicating the presence of a younger stellar population in the outer regions, albeit in a relatively small proportion. The overall morphology indicates minimal signs of recent or ongoing mergers or major disturbances.
