The galaxy presents as a spiral, viewed at an oblique angle. The central bulge appears relatively small and indistinct. A prominent disk is observed, displaying clear indications of spiral arm structure. The arms appear somewhat flocculent with regions of active star formation. Evidence of a bar structure is present but not prominent. The overall color suggests a relatively late-type spiral with ongoing star formation. There is also some indication of minor morphological disturbance, possibly due to a recent interaction or merger event, although no clear merger companion is visible. The galaxy has a blue hue. 