  A second galaxy ``missing dark matter" (NGC1052-DF4) has been recently
reported. Here we show, using the location of the Tip of the Red Giant Branch
(TRGB), that the distance to this galaxy is 14.2+-0.7 Mpc. This locates the
galaxy 6 Mpc closer than previously determined. We also analyse the distances
to the brightest galaxies in the field-of-view (FOV) of NGC1052. We find this
field is populated by two groups of galaxies in projection: one dominated by
NGC1052 and NGC1047 at ~19 Mpc and another group containing NGC1042 and NGC1035
(as well as [KKS2000]04 and NGC1052-DF4) at ~13.5 Mpc. At a distance of 13.5
Mpc the globular clusters of NGC1052-DF4 have the same properties than globular
clusters in the Milky Way and other dwarf galaxies.
