The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that appears yellowish-white in color, suggesting a population of older stars. There is a gradual fall-off in luminosity from the center outwards. The shape is close to circular, showing a slight ellipticity. No distinct spiral arms or dust lanes are discernible. There might be signs of a very faint disk, but the image resolution makes it difficult to confirm. There appears to be minimal to no morphological disturbance, such as tidal tails or signs of ongoing mergers.
