The galaxy presents as a relatively compact, elliptical morphology, exhibiting a smooth and largely featureless profile. The central region displays a pronounced concentration of light, appearing yellowish-white. A subtle color gradient is observed, with the outer regions transitioning toward a redder hue. No spiral arm structures or prominent dust lanes are discernible. The galaxy exhibits a degree of roundness, appearing more elliptical than spheroidal, but not highly elongated. There is no visual evidence of ongoing major mergers or significant tidal disturbances; however, the possibility of minor interactions cannot be ruled out at this resolution. The galaxy's color suggests a population of older stars and a relatively low star formation rate.
