The galaxy presents as a spiral galaxy, observed at a slight inclination. Two prominent spiral arms emanate from a central bulge, loosely wound around the galaxy. There does not seem to be a significant bar feature. The bulge appears moderately sized. Within the spiral arms, distinct regions of star formation are implied by the bluer concentrations, while older stellar populations are indicated by the yellowish glow of the bulge. There are no indications of strong tidal disturbances or a recent major merger, however, there may be some minor disturbances. The overall morphology suggests active star formation.
