The galaxy presents as a spiral type, viewed at an angle between face-on and edge-on. There is evidence of a central bulge, possibly of moderate size, with a disk extending outward. The spiral arms are somewhat distinct, indicating a barred spiral structure or possibly a disturbed morphology indicative of a past or ongoing interaction or minor merger. There are regions of enhanced blue coloration suggesting recent or ongoing star formation within the spiral arms. Redder areas are also visible, potentially indicative of older stellar populations or dust lanes. The overall shape appears somewhat elongated.
