The galaxy presents a distinct spiral structure. Two prominent spiral arms are visible, tightly wound around the galactic center. The central bulge appears relatively small and diffuse, with a yellowish hue suggesting an older stellar population. The spiral arms exhibit a bluer color, indicative of ongoing star formation. The disk component dominates the galaxy's morphology, with minimal indication of a bar structure. There is no strong evidence of any major merging event, although subtle disturbances in the disk's symmetry might suggest a minor interaction in the past.
