The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The central region displays a distinct yellowish hue, potentially indicative of an older stellar population dominated by redder giants and dwarfs. Moving outward from the core, the galaxy exhibits a gradual decrease in surface brightness, transitioning into a fainter, bluer halo. This halo appears relatively featureless, suggesting a lack of significant ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible, consistent with its classification as an elliptical or lenticular galaxy with minimal disk features. The object appears largely undisturbed, showing no clear signs of recent mergers or tidal interactions. Overall, the galaxy seems to be a massive and relatively quiescent system, with a substantial population of evolved stars.
