Left panels: velocity dispersion maps for the [O III], H₂[1-0 S(2)], and CO(1-0) emission lines (assuming a single Gaussian LOSVD) in the central 5″×5″ (∼3.5 kpc × 3.5 kpc) for [O III], H₂ and CO(1-0). The black contours indicate the [OIII] surface brightness distribution as a reference in all maps. The green cross marks the position of the AGN and the light blue contours represent the distribution of 10 GHz radio continuum emission as resolved with our VLA radio interferometric observations. The red circles indicates a circular aperture of 0.8″ in radius, which we use to extract spectra covering the two high dispersion region located south west and north east of the nucleus. Middle and right panels: spectra of the high dispersion regions in various emission lines from the optical, NIR and sub-mm observations for the south-west (middle) and north-east region (right). Most emission lines reveal an asymmetry towards the blue or red side that we model with two Gaussian line components, which we refer to as the core and wing component. Only Paβ and H₂[1-0 S(2)] can be well-described by only a single Gaussian component.