NGC 6764 is a composite galaxy exhibiting central activity ( LINER ) and recent massive star formation ( Wolf-Rayet galaxy ) .
We report new high-resolution interferometric data of the ^ { 12 } CO ( 1–0 ) and ^ { 12 } CO ( 2–1 ) emission in the central part of the galaxy together with high resolution VLA data of the radio continuum emission .
The bulk of molecular gas ( few times 10 ^ { 8 } { M _ { \odot } } ) is located in the central part .
A molecular outflow ( \sim 1.7 \times 10 ^ { 7 } { M _ { \odot } } ) out-of the plane is associated with the starburst-driven outflow radiocontinuum emission .