The object appears to be a spiral galaxy, viewed at an angle between face-on and edge-on. Evident dust lanes trace the spiral arms, which are somewhat flocculent in nature. There is some visual evidence of a central bulge, though it is difficult to determine the bulge size with precision. There is a faint bar structure spanning across the center of the galaxy. The overall structure appears relatively undisturbed, showing no obvious signs of ongoing major merging events.
