The galaxy presents as a disk galaxy, observed at a relatively high inclination. There is evidence of distinct spiral arm structure. There is an indication of a central bar feature crossing the nucleus. The arms appear somewhat flocculent, rather than tightly wound. The central bulge component appears to be small relative to the overall disk size, with a high fraction of the light coming from the disk. Patches of bluer light, suggestive of on-going star formation, are visible within the disk, particularly at the end of the arms. There is no obvious evidence of a major merger or significant tidal disturbance in the morphology.
