The galaxy presents as a spiral type, exhibiting a clear disk structure. Two prominent spiral arms emanate from the central region, tracing a grand design morphology. The winding of these arms appears intermediate, neither tightly wound nor particularly loose. A bar feature may be present, though it seems weak. The central bulge component is relatively small, and appears subdued. Star formation seems to be occurring, albeit at a modest rate, as can be inferred from the overall color. No major disturbances or signs of ongoing mergers are apparent.
