The galaxy exhibits a clear spiral structure with two prominent, well-defined arms. These arms are moderately wound, displaying a fairly tight morphology as they emanate from the central region. The nucleus appears as a bright, concentrated region. The galaxy displays a clear, well-formed disk shape. There is no apparent dust, although the arms have some blue tint which suggests the presence of hotter, younger stars. There are no apparent signs of tidal disturbance from recent or ongoing mergers. There may be a weak bar structure. The bulge is moderate in size.