The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, featureless appearance. The color profile indicates a dominant population of older stars, exhibiting a reddish-yellow hue. There is no apparent spiral arm structure or dust lane obscuration visible. The galaxy displays a high degree of circularity, with minimal elongation or tidal disturbances evident, suggesting it is not undergoing a major merger event. There is little sign of active star formation in this galaxy.