The galaxy presents a somewhat flocculent spiral structure, though the arms are not sharply defined. The disk appears to be oriented close to face-on. Hints of dust lanes and brighter star-forming regions are visible within the spiral arms. The central bulge is moderately sized and shows a relatively smooth profile. The galaxy displays a distinct blue coloration, suggesting the presence of a young stellar population. Based on its morphology, this is likely a late-type spiral galaxy undergoing active star formation. Some signs of possible minor interactions can be seen. The galaxy appears to be only slightly distorted.