The galaxy presents as a spiral type, viewed at an angle slightly off from face-on. Prominent spiral arms are visible, displaying a somewhat flocculent structure. The arms appear to originate from a central bulge. The bulge component is moderately sized. The spiral arms show evidence of ongoing star formation, indicated by the clumpy distribution of bluer light concentrations throughout the disk. The overall color of the galaxy is somewhat redder in the central regions, suggesting an older stellar population. There is little evidence of a strong bar structure within the galaxy. The morphology of the galaxy does not suggest any ongoing major merger activity, however there may be some minor disturbances in the outer regions. The disk extends a considerable distance from the bulge.
