Radial dependence of the rotating disk model parameters. Both model parameters of the galaxy stellar (blue) and ionized gas (blue) velocity field are shown. The data points acquired from the MUSE NFM-AO observations are shown as stars and have errors smaller than the size of the symbol. The data points from MUSE WFM are shown as errorbars. From to 25″, the PA of the disk-like rotation is constant and matches between ionized gas and stars. For both, the rotational velocity increases from the center up to ∼6″ before it flattens out.