The NGC 4485/NGC 4486 group is a small collection of galaxies located in the constellation Canes Venatici. This group primarily consists of two interacting galaxies, NGC 4485 and NGC 4486, which are notable for their gravitational interaction that can lead to star formation and other dynamic processes. NGC 4485 is a dwarf irregular galaxy, while NGC 4486 is a larger spiral galaxy. The interaction between these two galaxies provides valuable insights into the effects of gravitational forces on galaxy evolution and the formation of new stars in the universe.