The galaxy presents as a spiral type, with a disk structure. Spiral arms are clearly visible and extend outwards from the central region, exhibiting a somewhat grand design. The arms appear relatively open and loosely wound. There is some evidence of multiple arms. 

The central bulge appears relatively small and not particularly prominent. There may be a weak bar-like structure present in the central region, or some central asymmetry.

The galaxy appears to be undergoing some sort of interaction or disturbance, as suggested by an irregular shape. There may be a minor companion or a tidal feature suggesting a merger. The galaxy exhibits regions of active star formation within the spiral arms, indicated by a bluer hue. 
