Though this young open cluster is thought to contain more than a thousand stars, only about a hundred of these stand out against the background of the sky, primarily grouped towards the denser central regions of the cluster.
C75 (also designated NGC 6124) lies in the plane of the Galactic disc, at a distance of some 18,600 light years from the Solar System. None of its individual stars is brighter than magnitude +9, but collectively the cluster reaches a visual magnitude of +5.8. In principle this makes it bright enough to be seen with the naked eye, though only under absolutely ideal conditions.