In this image, the heart of the spiral galaxy M77 observed by ALMA (Atacama Large Millimeter/submillimeter Array) is superimposed on a visible light image taken by the Hubble Space Telescope. The distribution of cyanoacetylene (HC₃N) is shown in yellow; the distribution of carbon monosulfide (CS) in red; and the distribution of carbon monoxide (CO) in blue. Through ALMA observations, the existence of organic molecules concentrated around the supermassive black hole in the center of M77 was revealed for the first time.