This galaxy exhibits a generally smooth morphology, appearing somewhat elliptical in shape with a bright, concentrated central bulge. Surrounding the bulge is a fainter, more diffuse disk. The color gradient transitions from a yellowish-white core to a bluish-white periphery. This color suggests active star formation may be occurring in the outer regions. There are hints of minor disturbances in the galaxy's structure, but overall it appears relatively undisturbed. Evidence suggest a relatively high stellar mass.
