The galaxy presents as a centrally concentrated, ellipsoidal object with a smooth, relatively featureless morphology. The core region exhibits a bright, yellowish-white hue, suggesting a dominant population of older stars. The light intensity gradually diminishes outwards from the core, transitioning into a diffuse halo. There is no discernible spiral arm structure or prominent dust lanes visible. The galaxy exhibits a slightly elongated shape, appearing more rounded than cigar-shaped. No clear signs of ongoing major mergers or tidal disturbances are evident in this image, implying a relatively settled state. The observed color profile indicates a potential lack of significant recent star formation activity.
