The galaxy presents as a relatively smooth, elliptical-like structure. There is a central bulge that appears bright and concentrated. The light intensity gradually decreases from the center outwards, indicating a radial density profile. There is only a very faint hint of a disk and little discernible spiral arm structure or distinct star-forming regions, suggesting a largely quiescent system. The galaxy's overall color is moderately red, leaning toward yellow, implying an older stellar population. There appears to be a slight asymmetry to the galaxy’s overall shape, but with no indication of an ongoing major merger. The halo surrounding the galaxy is diffuse, indicating a smooth transition between the galaxy's main body and the intergalactic medium.