The galaxy presents as a spiral type, viewed at an oblique angle to its plane. Evidence of spiral arms exists, though they appear somewhat flocculent and not tightly wound. A central bulge is discernible, displaying a moderate size relative to the overall galactic disk, with a smooth appearance. Some areas of active star formation are suggested by the blue-ish color throughout the outer disk. Overall, the galaxy's disk appears relatively symmetric with only minor disturbances, and its structure suggests no current major merger activity.
