The galaxy presents a largely smooth morphology. It is an elliptical galaxy, with an apparent lack of spiral arm structures or significant dust lanes. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. The galaxy exhibits a slightly elongated shape, appearing more oblate than perfectly spherical. There is no strong evidence of ongoing mergers or major tidal disturbances. The overall color appears yellowish-white, indicative of an older stellar population with a lower rate of star formation.
