The galaxy presents a disk-like morphology. Prominent spiral arm structures are observed, exhibiting a relatively open winding. There appears to be some flocculence within the spiral arms. The central bulge is relatively small. No strong bar structure is apparent, although there may be a faint, weak central bar. There appears to be some form of disturbance visible. It is difficult to resolve if the disturbance is due to a minor or major merging event, or some other interaction. The overall color suggests a mix of stellar populations, with some bluer regions indicating ongoing star formation within the spiral arms, and a more yellow/red central region.
