Channel maps of ionized gas species tracing the outflow kinematics from MIRI and MUSE data. Upper panel: Channel maps of [Ne V] λ14 μm emission lines from MIRI data. Lower panel: Channel maps of [O III] λ5007 Å emission from WFM MUSE data. Contours indicate velocity dispersion levels of 97, 114, and 130 km s⁻¹ in the [Ne V] λ14 μm emission. Velocity bins are indicated at the top of every panel in kilometers per second and are computed relative to the same systemic velocity. The star marks the position of the nucleus based on the ALMA data (see Appendix A.3).