Stellar kinematic measurements extracted from the JWST/NIRSpec G235H/F170LP IFU. Panel A: Logarithmic integrated intensity collapsed along the spectral dimension (excluding the detector gap at ∼2.41–2.49 μm). Panel B: PPXF fit for the central VORONOI bin. Part of the central bin spectrum, which contains the stellar absorption features at ∼2.3 μm (CO band heads), is plotted in black, and the best-fit empirical X-shooter stellar library (XSL; Appendix A.1) is overlaid in red. The residuals (data-model) are illustrated in green. Two vertical gray lines indicate the spectral region where we actually fit the model templates to the spectra of all bins. Panels C, D, and E: Rotation (V), velocity dispersion (σ), and root-mean-squared velocity ($V_{\mathrm{rms}}=\sqrt{V^2+{\sigma }^2}$). White contours show the intensity, which decreases by 0.5 magnitudes from the center outward. We also performed the same measurements using the PHOENIX high-spectral-resolution synthetic spectral template (Appendix A.2), which are shown in Fig. A.1.