The galaxy presents as a face-on spiral, exhibiting two prominent, loosely wound spiral arms. These arms emanate from a central region, potentially hosting a small bulge. The overall color of the galaxy appears to be a bluish-white, suggestive of ongoing or recent star formation. The spiral arms are not uniform, and display clumpy regions that may correspond to star-forming regions or stellar associations. There is no indication of any major mergers or strong interactions with other galaxies. Based on its morphology, the galaxy appears to be a relatively isolated system with ongoing, though perhaps not extremely vigorous, star formation activity. The galaxy appears to be a regular spiral and not a barred spiral.