The galaxy appears to be a spiral type, presenting a disk-like structure viewed at a slight angle. The central bulge region exhibits a yellowish-white hue, suggestive of an older stellar population. The spiral arms are prominent and moderately wound, displaying a bluish tint indicative of ongoing star formation. The disk shows asymmetries, with a possible minor tidal disturbance on one side. The overall structure is consistent with a galaxy undergoing active star formation within its spiral arms, with a notable population of older stars concentrated in the central bulge. There is no apparent bar structure.
