The galaxy presents a discernible spiral structure, though not sharply defined. The arms exhibit a somewhat flocculent morphology, with regions of enhanced luminosity potentially indicating active star formation. The central bulge appears relatively small and indistinct. Overall, the galaxy's light distribution is suggestive of a disk-dominated system, although the smoothness observed may indicate the presence of an older stellar population within the arms. A slight asymmetry or minor disturbance is possibly present, without signs of major merging activity. The light distribution exhibits a slight elongation.
