The galaxy presents a generally smooth and centrally concentrated light profile, indicating a likely classification as an elliptical galaxy. Its shape appears moderately elliptical rather than perfectly spherical. There is little visible evidence of spiral arms or significant dust lanes. The galaxy exhibits a color gradient, appearing more yellow-reddish towards its core. The galaxy shows no signs of major mergers or tidal disturbances, suggesting it has likely been relatively undisturbed recently. It is a high mass galaxy, but the star formation rate appears to be low, and hence the galaxy is probably composed of old stellar populations. The galaxy is estimated to be several kiloparsecs in radius. 
