The isolated horizon formalism, together with a simple phenomenological mod
el for colored black holes was recently used to predict a formula for the A
DM mass of the solitons of the EYM system in terms of horizon properties of
black holes for all values of the horizon area. In this Brief Report, this
formula, is tested numerically-up to a large value of the area-for spheric
ally symmetric solutions and shown to yield the known masses of the soliton
s.