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In this proceeding we look at the relationship between the photometricnuclear properties of early-type galaxies from Hubble Space Telescope imagingand their overall kinematics as observed with the SAURON integral-fieldspectrograph. We compare the inner slope of their photometric profiles and theSlow/Fast rotator classes, defined by the amplitude of a newly defined LambdaRparameter, to show that slow rotators tend to be more massive systems anddisplay shallower inner profiles and fast rotators steper ones. It is importantto remark, however, that there is not a one-to-one relationship between the twophotometric and kinematic groups.

The kinematics of Core and Cusp galaxies: comparing HST imaging and integral-field observations