The galaxy presents a prominent spiral structure. Arms are clearly visible, with what appear to be two main arms. The spiral arms exhibit a moderately wound morphology, neither tightly coiled nor loosely extended. The image suggests it is a face-on spiral galaxy. A central bulge is present, though not the dominant feature of the galaxy. Evidence suggests the possibility of merging activity. It appears that a major disturbance is occurring on the spiral structure, with a smaller companion galaxy, and a likely ongoing merger. It exhibits distinct regions of star formation.
