This paper proposes a Symplectic Hamiltonian Graph Neural Network emulator for softened gravitational N-body dynamics. Instead of learning a direct state-to-state map, the method learns a separable Hamiltonian $H(q,p)=T(p)+U(q)$, where $T$ is analytic and $U(q)$ is parameterized as a permutation-invariant sum over pairwise interactions computed by an MLP on softened distances (Sec. 2.2, Eq. (1)–(3)). Forces are obtained by automatic differentiation, ensuring a conservative force field. A differentiable leapfrog (kick–drift–kick) integrator is unrolled in training so the learned discrete-time flow is symplectic by construction for the learned separable Hamiltonian (Sec. 2.3). Experiments train on $N=50$ virialized Plummer spheres generated with softened gravity and leapfrog integration, using rotation/translation augmentation and a two-stage radial curriculum that initially masks the dense core (Sec. 2.1, Sec. 2.3). Evaluation reports trajectory reconstruction error and tests for physically meaningful behavior (bounded energy error, time reversibility, and a numerical Jacobian-determinant-based volume check) and includes zero-shot transfer to $N=25$ and $N=100$ (Sec. 3.1–3.2). The overall direction is well-motivated, but the manuscript currently underspecifies the architecture/training and relies on weak baselines and largely qualitative reporting; several claims (novelty/positioning, symplecticity verification, and breadth of “generalization”) need tightening and/or stronger experiments to be fully convincing.