The galaxy presents as an elliptical morphology, exhibiting a generally smooth and centralized luminosity profile. It appears to be moderately rounded. The color gradient suggests a relatively older stellar population. The central region displays a yellowish hue, possibly indicative of a concentration of evolved stars. There is no discernible spiral arm structure or dust lane obscuration. The galaxy exhibits no signs of a major ongoing merger, though a minor disturbance may be present. There is a low rate of star formation. The galaxy is a significant mass.
