Voronoi binned stellar velocity maps for the F170LP NIRSpec observations. The four panels show the line-of-sight velocity (V), the velocity dispersion (σ), and the first two Gaussian-Hermite moments (h₃ and h₄). The black diamonds show the five masked spaxels where a stellar fit is not possible due to the strong non-thermal AGN continuum. The orientation is the same as that in Figure 10.