The galaxy presents as a moderately bright, elliptical-like structure with a smooth, featureless appearance. Its core exhibits a concentrated, yellowish-white luminosity, suggestive of an older stellar population. The color gradient shifts subtly outwards, displaying a slightly reddish hue at the edges, which could be indicative of dust lanes or cooler stars. The shape is more elongated than circular but not extremely so; its axial ratio suggests an intermediate ellipticity. There is no visual evidence of spiral arms, a prominent disk, or active star formation regions. The galaxy does not appear to be undergoing a major merger, but subtle disturbances cannot be ruled out based solely on visual inspection of this image.
