The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a slight elongation, suggesting a deviation from perfect sphericity. The core exhibits a yellowish hue, potentially indicative of an older stellar population. The galaxy appears largely undisturbed, with no readily apparent signs of major mergers or significant tidal interactions. The light smoothly decreases from the core to the edge, and lacks prominent spiral arm features or significant dust lane obstructions. 
