The galaxy appears as a centrally concentrated, elliptical structure with a smooth light distribution. The core is bright, exhibiting a yellowish-orange hue, which may indicate a population of older stars. There is no discernible spiral structure or distinct features like dust lanes or active star-forming regions. The isophotes appear relatively round, indicating a low ellipticity. No signs of tidal disturbances or interactions with other galaxies are immediately apparent in the image. The overall color suggests a relatively passive galaxy with a low star formation rate.
