The galaxy presents a predominantly smooth morphology, appearing elliptical in shape. It exhibits a radial color gradient, with a yellowish-white core that transitions to a bluish-white outer halo. The galaxy shows limited signs of ongoing mergers or major disturbances, although subtle irregularities in the outer halo might suggest minor past interactions. There are hints of a disk-like structure embedded within the smoother, elliptical profile, which is potentially indicative of a spiral galaxy that is being viewed at an angle. The overall structure suggests a mature galaxy with a significant stellar mass.
