Morpho-kinematic analysis for cluster galaxy #10. Top row on the left: HST/ACS F814W image. Top row in the middle: Galfit model (exponential + de Vaucouleurs profile). Top row on the right: Galfit residuals. Second row on the left: MUSE HαS/N map, as measured with MPDAF. Second row in the middle: MUSE Hα flux map, as measured with MPDAF, in units of 10⁻²⁰ erg s⁻¹ cm⁻² arcsec⁻². Second row on the right: modelled Hα flux map from GalPaK3D, in the same flux units as before. Third row on the left: MUSE Hα velocity map, in units of km s⁻¹ as measured with MPDAF. Third row in the middle: modelled Hα velocity map in km s⁻¹ from GalPaK3D. Third row on the right: modelled Hα velocity profile from GalPaK3D. Last row on the left: MUSE Hα velocity dispersion map, in units of km s⁻¹ as measured with MPDAF. Last row in the middle: Modelled Hα velocity dispersion map in km s⁻¹ from GalPaK3D. Last row on the right: modelled Hα velocity dispersion profile from GalPaK3D. This galaxy is classified as being morphologically and kinematically regular. It has the following physical parameters: log(M/M_⊙) = 8.74; v_max = 98 km s⁻¹; v_max, gas/σ_gas = 3.03; offset from star-forming MS: Δ_MS = 0.1; offset from TFR: ΔM_TFR = 0.27; offset from stellar mass–S_0.5: ΔM_S0.5 = 1.0.