The galaxy presents as a somewhat diffuse, face-on spiral. It exhibits a central bulge region that appears relatively small and not particularly prominent. The spiral arms are not well-defined, appearing patchy and somewhat flocculent in nature. There is evidence of ongoing star formation, indicated by the presence of bluer regions, primarily within the disk component and along the indistinct spiral arms. The overall color suggests a mix of stellar populations, with a possible dominance of older, redder stars in the bulge, contrasted by the younger, bluer stars in the disk. No significant dust lanes are clearly visible. The morphology appears slightly disturbed, which could be indicative of a minor interaction or merger event in its past or present.
