The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification or a spiral galaxy viewed face-on without prominent spiral arm structure. The central region exhibits a high concentration of luminosity, indicative of a substantial bulge or a bright active galactic nucleus. The overall color appears relatively red, leaning toward a yellow hue. Given its apparent color, this galaxy likely contains a significant population of older stars. The galaxy appears generally round, although it may be slightly elongated. There's no obvious indication of ongoing major mergers or significant tidal disturbances.