The galaxy presents as a generally smooth, elliptical-like structure, with a high degree of central concentration of light. The overall shape appears to be somewhere between round and cigar shaped. There is no immediately obvious disk or spiral structure, and no visual indications of any major or minor mergers. It appears as a relatively isolated galaxy. The galaxy exhibits a color gradient, shifting from a yellow-white hue at its core to more reddish tones in its outer regions. This indicates the presence of older stellar populations in the central bulge and relatively little current star formation. The outer regions are fainter and more diffuse, suggesting lower stellar density and potentially a halo of older stars. The galaxy's color is overall relatively red, suggesting older stars are dominant.
