Stellar and ionised-gas analysis for FCC 179. First row panels: MUSE reconstructed image (left). The dotted ellipse corresponds to the isophote at μ_B = 25 mag arcsec⁻². Maps of the mean velocity (middle) and velocity dispersion (right) of the stellar LOSVD. Second row panels: radial profiles of the kinematic (black circles) and photometric (green circles) position angle (left). The vertical dashed lines mark the radial range where the average position angles are computed. Maps of the third (middle) and fourth Gauss-Hermite coefficient (right) of the stellar LOSVD. Third row panels: map of the ionised-gas classification (right) into H II regions (blue), highly-ionised or AGN regions (yellow), LINER-like emission regions (red), and regions where the nebular emission is powered by some combination of massive-star radiation and other ionisation sources (green).