The galaxy presents a clear spiral structure. Two dominant spiral arms are easily discernible, winding moderately around a central bulge. The arms appear relatively symmetrical. The bulge size is of moderate proportion to the disk. Star formation seems present, with the arms displaying hints of clumpy regions, potentially indicative of HII regions. The galaxy does not exhibit obvious signs of major mergers or significant tidal disturbances. The galaxy is not edge-on but is instead viewed with a clear view of the plane. There are no obvious signs of a strong bar structure.
