The galaxy appears as a relatively smooth, centrally concentrated elliptical object. It exhibits a moderate degree of ellipticity, appearing more oblate than perfectly spherical. The color profile suggests a population of older stars, with a yellowish-red hue dominating the galaxy's overall light. There's no readily apparent evidence of spiral arms or significant dust lanes within the resolution afforded by the image. The morphology indicates it's a relatively undisturbed system, with no major signs of ongoing or recent mergers.
