This galaxy presents a spiral morphology, observed at a moderate angle relative to edge-on. Prominent spiral arms are clearly visible, exhibiting a tightly wound structure. These arms are well-defined and exhibit a patchy distribution of star formation regions, indicated by their slightly bluer color.

The central bulge appears relatively small compared to the overall disk size. A bar-like structure is present in the central region, appearing somewhat subtle. The disk appears largely undisturbed, showing no apparent signs of major merging activity or significant tidal distortions, though some minor asymmetric features are present. The overall color of the galaxy appears to be relatively consistent, with a slight reddening towards the central bulge, which indicates an older stellar population.
