  We report on an old computation of propagators of massless scalar fields on
an ensemble of configurations in the 4D path integral of Euclidean dynamical
triangulations in the collapsed (crumpled) phase. The resulting quantum average
is used to calculate the scale factor of a rotational invariant metric in a
4-dimensional space. This new scale factor is non-zero at the origin, which we
assume to be caused by the presence of the well-known singular structure in the
collapsed phase. It depends on an overall integration constant. A
transformation to a metric in (1+3)-dimensions reveals Euclidean black hole
features at an instant in time, with a horizon separating interior and exterior
parts. Effective Einstein equations in the presence of a `geometric condensate'
are assumed, and computed with the software OGRe. We find similarities with the
energy density and pressure of gravastars, as well as remnants, and investigate
their dependence on the integration constant.
