The galaxy presents a distinct spiral morphology. Two prominent spiral arms are observed, exhibiting a loosely wound structure extending from the central region. The central bulge is visible, and appears to be of moderate size. The galaxy displays a disk-like structure, and is viewed face-on. No significant bar structure is observed. The overall structure appears to be relatively undisturbed, with only subtle signs of minor interaction or merging activity. Star formation appears to be ongoing within the spiral arms.
