  We present results from our ongoing effort to understand the morphological
and kinematical properties of early-type galaxies using the integral-field
spectrograph SAURON. We discuss the relation between the stellar and gas
morphology and kinematics in our sub-sample of 24 representative Sa spiral
bulges. We focus on the frequency of kinematically decoupled components and on
the presence of star formation in circumnuclear rings.
