The galaxy presents a concentrated, bright central bulge, which is ellipsoidal in shape. A faint disk component is suspected surrounding the central bulge, although it is difficult to distinguish discrete spiral arm structures. The color profile indicates an older stellar population, particularly within the bulge, as evidenced by the reddish-yellow hue. There is a slight indication of a disturbance on the outskirts of the disk; but overall the morphology is relatively undisturbed.
