The galaxy presents as a spiral type, with a defined, yet compact structure. The spiral arms are tightly wound, exhibiting a flocculent morphology. They appear somewhat fragmented, hinting at ongoing or recent star formation within the arms themselves. The central bulge is relatively small, and not especially luminous. There is little evidence of a bar structure within the galaxy's core. The overall color is predominantly bluish, indicative of a relatively young stellar population. The spiral arm structure dominates the galaxy's appearance, with little visible evidence of interaction or major disturbances. It is a well-defined spiral galaxy.
