NGC 4676B is a galaxy located approximately 100 million light-years away in the constellation Coma Berenices. It is part of a pair of interacting galaxies known as the Mice Galaxies, which also includes its companion, NGC 4676A. The interaction between these two galaxies is causing significant distortions in their shapes and triggering new star formation. This galaxy is classified as a spiral galaxy and exhibits features typical of galaxies undergoing gravitational interactions. The ongoing merger process between NGC 4676B and NGC 4676A provides valuable insights into the dynamics of galaxy evolution and the effects of galactic collisions on star formation rates.