The galaxy presents as a relatively small, edge-on spiral. The disk is thin and appears to be mostly smooth, with no obvious signs of spiral arm structure or dust lanes visible in this image. There is no prominent bulge component observed. The galaxy appears relatively undisturbed, showing no signs of a recent major merger event. A very slight asymmetry is visible in the outer edges of the disk, suggesting the possibility of a minor interaction or internal disturbance. Overall, the galaxy seems to be a relatively quiescent disk galaxy.
