The galaxy presents a distinct spiral morphology with a central bulge. The spiral arms are prominent, loosely wound and appear bifurcated, suggesting a two-armed spiral structure. The bulge appears relatively small compared to the overall disk size, showing a moderate contribution to the galaxy's total light. There is evidence of ongoing star formation within the spiral arms, indicated by the presence of bluer regions and possibly HII regions. No significant dust lanes are readily apparent. A slight asymmetry in the spiral arm structure might indicate a minor gravitational interaction or internal disturbance within the galaxy. The disk is oriented somewhat face-on, allowing for detailed examination of its spiral structure.