The galaxy presents as a spiral type. Distinct spiral arms are visible, extending from a central bulge. The arms exhibit a moderate winding pattern and are somewhat fragmented in appearance. There appears to be two dominant spiral arms. The central bulge has a yellowish hue, potentially indicating an older stellar population. The spiral arms show a bluer tint, suggestive of ongoing star formation. There appears to be a possible ongoing merging event on the left side of the galaxy.
