The galaxy presents a generally smooth and rounded morphology. Its color profile is characterized by a central reddish hue that gradually transitions to a greenish-yellow at the periphery. The relative lack of discernible structural features, such as spiral arms or a prominent disk, suggests that it is not a spiral galaxy. There are no signs of major tidal disturbances or ongoing mergers. The galaxy exhibits a notable diffuse quality and lacks the sharp definition associated with younger stellar populations. The roundness of the galaxy suggests it is not a disk dominated galaxy.