The observed galaxy presents as a spiral structure, with the majority of citizen scientists agreeing on this classification. It displays a prominent disk with a defined spiral arm morphology. The spiral arms appear to be largely two in number, with a moderately wound appearance. The central bulge is moderate in size relative to the disk, and the overall color indices indicate a relatively high rate of star formation. There is no strong visual evidence of a bar structure. Analysis of the image also suggests a possible minor disturbance, with an overwhelming consensus stating no merging is actively occurring.
