The galaxy presents a prominent disk structure with a notable spiral arm morphology. The spiral arms appear well-defined, extending outwards from a central bulge. The bulge appears moderate in size, and the disk shows a subtle inclination relative to the observer's line of sight, but is still more face on. A bar appears present, with moderate strength. There is no apparent major merger or extreme disturbance in the galaxy's structure, but a minor merger cannot be ruled out. The colour gradient suggests a mix of stellar populations, with bluer regions likely indicating ongoing star formation. The overall smoothness suggests it is not an elliptical galaxy.
