The galaxy exhibits a morphology suggestive of a spiral type, though the resolution limits a definitive classification. There is a noticeable central bulge, estimated to be moderate in size relative to the overall galactic structure. Faint spiral arm structures appear to emanate from the central region, displaying a somewhat flocculent and not highly organized pattern. The disk appears to be viewed at an angle close to face-on. Some regions of potential star formation are subtly highlighted by bluish hues. Overall, the galaxy exhibits a somewhat disturbed morphology possibly indicating past or current interactions.
