The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. There is little evidence of spiral arm structures or dust lanes; the overall morphology appears quite regular. The galaxy presents an oblate shape. The color profile suggests a population of older stars, with the presence of a more yellow hue. There are no obvious signs of active star formation in the image. There is no visual evidence of tidal disturbances or interactions with other galaxies.
