Morphology and stellar kinematics of the sample galaxies. For each galaxy the top panel shows the galaxy image. The slit position and image orientation are indicated. The inset shows the portion of the galaxy image marked with a black box. The gray scale and isophotes were chosen to enhance the features observed in the central regions. The remaining panels show from top to bottom the radial profiles of h₄, h₃, σ_los, and velocity v (obtained by subtracting the systemic velocity from v_los). The best exponential fit to the σ_los radial profile is also shown by a black solid line in the corresponding panel.