The galaxy presents as a centrally concentrated object, characterized by a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white hue, indicating a high concentration of older stars. This central bulge gradually transitions into a fainter, more diffuse outer region. There appears to be a slight reddish tint surrounding the yellowish central core, suggesting the presence of a population of stars in a later stage of stellar evolution. The overall structure lacks any prominent spiral arms or distinct features, consistent with an elliptical galaxy classification. There are no signs of active galactic nuclei or significant dust lanes visible in this image. The galaxy exhibits a high degree of roundness. Furthermore, the morphology appears undisturbed, showing no obvious signs of recent mergers or tidal interactions.
