Kinematics of the stars and gas. Top row: MUSE stellar kinematics. Centre row: MUSE Hα kinematics. The black box in the bottom right corner indicates the position of what we interpret as an extraplanar Hα cloud. Bottom row: molecular gas kinematics from ALMA CO(2-1) (mom1 and mom2 maps). The footprint of the MUSE data is overlaid in black. All velocity maps have been corrected for systemic velocity; no inclination correction has been applied. The velocity dispersion maps refer to the intrinsic dispersion (instrumental effects have been removed). The white dashed lines sketch the position of the bar and spiral arms as shown in Fig. 1 (see Sect. 1). A zoom-in into the central kinematics is shown in Fig. 11.