The galaxy presents as a spiral galaxy, with a notable disk component. The spiral arms are somewhat flocculent in nature. The central bulge region appears prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk demonstrates a bluer color, indicative of ongoing star formation. There is a faint bar-like structure visible traversing the central region, though not particularly strong. There is no major morphological evidence of a significant merger event. The overall morphology suggests a moderately massive galaxy.