The galaxy exhibits a generally smooth morphology with a somewhat diffuse appearance. It appears to be an elliptical galaxy, but there is significant disturbance that suggests a major merger or interaction, it has a round shape with an axis ratio indicating that it is close to face-on. The color profile of the galaxy shifts from slightly bluer hues in the outer regions to a redder core, which is indicative of an aging stellar population. The galaxy is a relatively low redshift, meaning that it is relatively close to us. It has a relatively high mass and low star formation rate.