The galaxy presents as a spiral type, showing discernible spiral arm structures. The arms appear somewhat patchy and not uniformly distributed around the central bulge. The central bulge is moderately prominent, but not dominant. Some arms appear to be ill-defined, lacking crisp boundaries. There is evidence of active star formation within the spiral arms, indicated by regions with a bluer hue. The disk appears to be viewed at an angle that is far from edge on. There is no strong indication of a bar structure, but a mild asymmetry or disruption in the galactic disk might be visible. No clear merger is visible.
