The observed galaxy presents as a spiral type. The galaxy displays a prominent disk structure, which appears to dominate the visual morphology. Within the disk, evidence of spiral arms is detected, though they appear somewhat tightly wound. There appears to be moderate star formation activity. I do not detect any strong visual signs of an actively merging system, although there does appear to be a minor disturbance present. The bulge is subtle and small in size. The disk is oriented face-on relative to our line of sight. I see no strong evidence for a bar structure.
