The galaxy presents as a centrally concentrated, relatively smooth system. Its overall shape is elliptical, appearing somewhat rounded but trending towards a slightly elongated form. The light profile indicates a centrally bright core that diffuses outwards, with a gradual decrease in luminosity towards the edges. There is little evidence of distinct spiral arms or significant dust lanes. Minor disturbances or subtle irregularities are not strongly apparent in this image, however, there seems to be minor interaction with a galaxy above. The galaxy's color suggests a population of older stars, indicated by a relatively red hue.
