The galaxy presents as a moderately bright, non-edge-on spiral with indications of discernible, though somewhat tightly wound, spiral arms. The central bulge appears moderate in size. Some asymmetry is observable in the outer regions, possibly suggesting minor disturbances or tidal interactions. The disk exhibits a color gradient, appearing bluer towards the periphery and redder in the central region. The galaxy shows a central concentration with a somewhat smooth appearance, the disk shows some clumpy areas. Bar structure is likely present, as its light is more diffused. There appears to be a small amount of merging occurring.
