The galaxy presents as an elliptical or lenticular type, appearing largely smooth and homogenous in structure. There is no discernible spiral arm structure or prominent dust lanes. Its overall color is yellowish-white, suggesting a population of older stars and a relatively low rate of ongoing star formation. The galaxy exhibits a high degree of circularity, with only a slight deviation from a perfectly rounded shape. There is no obvious indication of any significant tidal disturbances or ongoing major merger events. Faint hints of a possible minor disturbance or interaction can not be ruled out. It appears as a non-active galaxy with a low star formation rate. The galaxy is estimated to be of intermediate mass.
