The galaxy presents as a generally smooth, elliptical-like structure. The light distribution appears highly concentrated towards the center, with a radial falloff in brightness. The galaxy exhibits a yellowish-red color, which may indicate an older stellar population or a significant dust component. There are no easily discernible features such as spiral arms or a prominent disk component. It exhibits a high degree of circularity. There are no visible signs of any major ongoing merger activity or significant tidal disturbances.
