The galaxy presents as a spiral type, with a prominent disk structure. The disk exhibits a discernible but somewhat flocculent spiral arm morphology, characterized by patchy regions of enhanced luminosity and a relatively high degree of openness. A central bulge is visible, though it appears moderately sized relative to the overall disk. The bulge exhibits a color gradient shifting towards redder hues than the disk, suggesting an older stellar population. Fainter spiral arms are visible extending outwards from the central disk, as well as a relatively small bar-like structure in the very center. 
