Canes Venatici II Group
The Canes Venatici II Group is a group of galaxies with a large collection of spiral
galaxies, the dominant members are which are probably M106, NGC 4096,
and NGC 4490. It lies at an average distance of 22 million light-years in
the constellation Canes Venatici, directly behind
the Canes Venatici I Group.
|M106 and possible companion spiral
NGC 4217 (lower right)