The galaxy presents as a spiral type, displaying a well-defined disk structure. High degree of dust and gas content apparent via color. The arms are tightly wound around a small, yet discernible central bulge, possibly indicating a relatively older stellar population residing in the core. Although there is some central light, it is relatively small. There are multiple well defined spiral arms, with some clumpy sections. Based on morphology, the most likely explanation is ongoing star formation. It shows no signs of major disturbances or ongoing mergers, although the elongated tail on the right of the disk could be the result of a minor interaction. Overall, the galaxy seems to be relatively undisturbed, and likely has high star formation.