The galaxy appears to be a spiral galaxy exhibiting a prominent disk structure. The spiral arms are well-defined and appear somewhat loosely wound, extending outwards from a central bulge. Within the spiral arms, clumpy regions of brighter light are visible, suggesting areas of active star formation. The central bulge appears relatively small. There is evidence of a bar-like structure across the center of the bulge. The overall color of the galaxy is blue, indicative of a significant population of young, hot stars. The galaxy appears somewhat disturbed, perhaps from a minor interaction with a nearby galaxy, but is mostly not merging.
