The galaxy presents a spiral morphology. Two clearly defined spiral arms appear to originate near the central bulge and extend outwards. The arms appear to be moderately wound. The galaxy exhibits a prominent central bulge. The disk is oriented at a small inclination, with a nearly face on view. There is no obvious bar structure visible in the image. Overall, the galaxy appears relatively undisturbed with no major signs of merging, although it appears to have a somewhat asymmetric morphology. The color gradients suggest ongoing star formation.
