The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its color gradient indicates a likely evolved stellar population, with a yellowish-orange hue dominating the central regions, suggesting older, cooler stars. A slight transition to a bluer tint in the outer regions may indicate the presence of younger stars, but these features are not pronounced. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal distortions. The overall shape is moderately elongated. Evidence of recent star formation appears to be minimal.
