NGC 4676A is a spiral 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 4676B. The interaction between these two galaxies is causing significant distortions in their shapes. This galaxy is notable for its bright, elongated structure and the presence of star formation activity triggered by the gravitational forces at play. Observations of NGC 4676A provide valuable insights into the processes of galaxy evolution and the effects of galactic interactions on star formation.