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We present surface photometry and stellar kinematics of NGC 4264, alenticular galaxy in the region of the Virgo Cluster undergoing a tidalinteraction with its neighbour, NGC 4261. We measured the bar radius andstrength from SDSS imaging and the bar pattern speed from MUSE integral-fieldspectroscopy. We find that NGC 4264 hosts a strong and large bar, which isrotating fast. The accurate measurement of the bar rotation rate allows us toexclude that the formation of the bar was triggered by the ongoing interaction.

A MUSE study of the fast bar in the weakly-interacting galaxy NGC 4264