The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated spheroid of light. The color profile suggests a population of older stars, indicated by the yellowish hue. There's a subtle hint of a disk structure, but the dominant feature is the bulge. No strong evidence of spiral arms or significant dust lanes is apparent in this image. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions, although there may be a very minor disturbance. There also seem to be some very minor tidal features present. The central region exhibits a bright core, potentially indicating the presence of an active galactic nucleus or a high concentration of stars.
