The galaxy presents as a fairly smooth, elliptical-like structure. Its light profile appears centrally concentrated, with a gradual decrease in luminosity moving outward from the core. The central region exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter blue emissions are observed in the galaxy's surrounding regions. There is no obvious spiral structure, disk, or dust lane, however, this could be due to the image quality. The galaxy's overall shape is closer to 'in between' circular and elongated. There is no indication of any major mergers or significant tidal disturbances. The galaxy appears relatively isolated with no obvious interacting companion.
