The galaxy exhibits an elliptical morphology, appearing largely smooth and featureless. It presents a concentrated central bulge, decreasing in luminosity outwards. The galaxy displays a slight elongation. The color gradient suggests an older stellar population dominating the light emission, appearing more red in the central regions. Little evidence of spiral arm structure or significant dust lanes is visible. The galaxy appears relatively isolated and undisturbed in its immediate vicinity. The overall appearance suggests a galaxy that has undergone significant aging of its stellar populations, with a relatively low ongoing star formation rate.
