We present gaseous and stellar kinematics for 14 gas-rich early-type galaxies. Half of the galaxies show irregular gaseous velocity profiles, with gas/star counter-rotation in 5 galaxies. We also find 5 counter-rotating stellar cores, and 5 more galaxies display stellar nuclei kinematically decoupled from the main stellar body. Our results indicate that the ionized gas is of external origin, and may have been acquired recently; the merging or accretion events that brought the gas into the galaxy have likely affected its stellar kinematics.