The galaxy presents as a spiral morphology, although the spiral arms are not sharply defined, appearing somewhat flocculent. The central bulge appears moderately prominent. The galaxy's disk exhibits a blueish tint, suggestive of recent or ongoing star formation, and regions of enhanced star formation appear clumpy. The overall color indices suggest a relatively actively star-forming galaxy. The galaxy does not display any major signs of ongoing mergers or significant tidal disturbances, though a slight asymmetry in the disk could indicate a minor interaction in the past.
