The galaxy presents as a generally smooth, elliptical object with a reddish-yellow hue, indicative of an older stellar population. The galaxy appears to be undergoing a minor interaction, as evidenced by a slight disturbance or asymmetry in its morphology. The galaxy seems to have a concentrated bulge and a moderately bright core. There is a secondary concentration of light close to the galaxy. Its overall structure suggests a relatively low star formation rate. The galaxy appears to be quite massive. 
