  We present surface photometry and stellar kinematics of NGC 4264, a
lenticular galaxy in the region of the Virgo Cluster undergoing a tidal
interaction with its neighbour, NGC 4261. We measured the bar radius and
strength from SDSS imaging and the bar pattern speed from MUSE integral-field
spectroscopy. We find that NGC 4264 hosts a strong and large bar, which is
rotating fast. The accurate measurement of the bar rotation rate allows us to
exclude that the formation of the bar was triggered by the ongoing interaction.
