The galaxy presents as a disk galaxy, viewed at an intermediate inclination. A bulge is visible in the center of the galaxy, appearing approximately yellow-orange in color. The disk component is characterized by spiral arm structures that appear somewhat flocculent and patchy. The disk exhibits a bluer color profile than the bulge, potentially indicative of ongoing star formation activity within the spiral arms. Some slight asymmetry can be observed in the disk, perhaps due to minor gravitational interactions or internal dynamics. There are no obvious signs of a major ongoing merger event.
