We present new radio continuum, 21 cm HI, 2.6 mm CO, and optical data for the NGC 4410 galaxy group, and compare with available X-ray maps. This group contains the peculiar radio galaxy NGC 4410A, which has a distorted double-lobed radio structure. NGC 4410A is strongly interacting with three nearby galaxies, and has a peculiar ring-like optical morphology, a number of extremely luminous H II regions, as well as tidal tails and bridges variously visible in optical, HI, and X-ray light. In this poster, we discuss how the gravitational interaction has affected the interstellar matter, the star formation rate, and the radio lobes in this system.