The galaxy presents as a single, concentrated object with a smooth and somewhat elliptical morphology. The core region is characterized by a bright, yellowish-white hue, suggesting a high concentration of older stellar populations. The galaxy appears relatively undisturbed, showing no obvious signs of tidal features, strong spiral arms, or other indicators of recent mergers or significant interactions. The galaxy’s outer regions exhibit a subtle fading of the yellowish hue into a more reddish tone, possibly indicating the presence of a population of evolved, redder stars. The overall light distribution indicates a relatively uniform stellar population. No significant dust lanes or prominent star-forming regions are visible within the galaxy.
