The AGORA Collaboration's latest preprint (arXiv:2605.24097) introduces a halo-tracking method via Haskap Pie that treats dark matter structures as intrinsically non-spherical, applied to the CosmoRun suite of hydrodynamic simulations run across multiple codes. Methodology involved bound-particle searches on merger histories, tracking shape metrics like axis ratios and spin without assuming virialized spheres; sample encompassed several high-resolution zoom-in runs but lacked direct observational calibration. As a preprint, findings await peer review. This approach reveals merger-driven spikes in morphological measures that single-code studies routinely miss, with timing discrepancies between simulations amplifying differences in pre-merger dynamical states. Secular trends show halo spin and major-to-minor axis ratios peaking at 4>z>2 then declining, while overdensity diverges for low-mass halos at low redshift—patterns tied to departures from the Virial Theorem. Prior AGORA papers (e.g., arXiv:1509.05848 on code comparisons) and IllustrisTNG analyses (e.g., arXiv:1707.03395) assumed spherical symmetry, underestimating how high mass-ratio mergers reshape halos and propagate errors into all semi-analytic galaxy formation prescriptions. The deeper pattern is that these morphology issues are not code-specific artifacts but systemic, demanding revisions to models reliant on spherical collapse approximations.