Estimates of the cluster's true diameter vary between about forty and ninety light years, and within this region hundreds of stars are densely packed, including a large number of variable stars. The cluster lies close to the plane of the Milky Way, and so - as viewed from Earth - its light is dimmed somewhat by intervening gas and dust from the Galactic disc. If it lay farther from the band of the Milky Way, C105 would shine more brightly in the skies of Earth.