The galaxy presents a clear spiral morphology. Two prominent spiral arms originate from the central bulge, winding relatively tightly around the galaxy's core. The arms exhibit a mottled appearance, suggesting regions of star formation or dust obscuration. The central bulge appears luminous and moderately sized compared to the overall galactic structure. The disk demonstrates a slight ellipticity, with an approximate major to minor axis ratio of 5:4. There is no strong evidence of a bar feature. The galaxy's overall color profile suggests a mix of stellar populations with varying ages, as blue hues are observed within the arms contrasting with the redder core. There appear to be only minor disturbances, with no strong signs of on-going merging.