The galaxy presents as a spiral type with a prominent central bulge. The bulge appears moderately sized, contributing significantly to the overall luminosity. There is evidence of spiral arm structure, although the arms are not tightly wound and display a somewhat flocculent or patchy morphology. A bar feature is suspected, with a subtle elongation extending across the central region of the galaxy. The disk appears to be viewed close to face-on. There is no obvious major merger, or signficant disturbance in the morphology, although some minor disturbances cannot be ruled out. Overall it is a spiral with moderately sized bulge, with flocculent arms that are slightly elongated.