The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There is an absence of clearly defined spiral arms or prominent dust lanes. The color profile suggests a population of older stars, with a reddish hue dominating the outer regions, transitioning to a slightly brighter, yellower core. The galaxy appears nearly edge-on, with a minor axis only slightly smaller than its major axis. The overall form appears largely undisturbed, showing no strong signs of recent major merger activity, though there is a slight asymmetry in the isophotes. The galaxy exhibits a high degree of central concentration.