We compute the third-order Bondi shear in the null surface formulation (NSF) of general relativity with definite graviton helicities. The quantum operator is derived explicitly in terms of the four helicity channels (I)–(IV) of the scattering equation, and compared with the helicity-summed result of Ref.~\cite{PRL2026}. Applied to two-graviton scattering, the contribution for the process generates simultaneously the - and -channel poles of the tree-level graviton amplitude. An explicit Wick-contraction calculation (Appendix~\ref{app:Wick}) shows that the NSF kernels yield \begin{equation*} ^{(33)}\big|_{(+,-\to+,-)} = 16πG,\frac{s^3}{tu}, \end{equation*} from first principles, with the angular integration over manifestly finite and no propagator introduced. The pole structure and the dependence are exact consequences of the null-cone geometry; the coefficient follows from the Ashtekar normalization of the asymptotic modes, in analogy with Ref.~\cite{PRD2026partI}. Both - and -channel poles arise simultaneously from a single Wick contraction; in covariant perturbation theory they arise from two separate Feynman diagrams. The completion of the tree-level amplitude via is carried out in Part~III~\cite{PRD2026partIII}. Unitarity at order is verified; the operators are identified as the terms of the Baker-Campbell-Hausdorff expansion of , establishing unitarity as a structural consequence of the recursive NSF equations~\cite{SmatrixNSF}.

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