Maps of the surface brightness, Σ (left column), velocity, V (middle column), and velocity dispersion, σ (right column) measured for [O III] λ5007 (upper row) and [Fe VII] λ6087 (lower row), respectively. The grey contours indicate the stellar continuum estimated in the range between λ = 5250 Å and λ = 5450 Å in the rest frame of the galaxy. The black contours correspond to the unresolved 8.49 GHz radio emission from NVAS with a beam size of $0\stackrel{″}{.}36\times 0\stackrel{″}{.}22$ and a position angle of $\mathrm{PA}=-19\stackrel{°}{.}93$. The separation between contours corresponds to factors of two in surface brightness. The purple circle indicates the FWHM of the MUSE data, $0\stackrel{″}{.}08$. The cross indicates the centre of the galaxy. The axes labels are in arcseconds. North is up and east is to the left.