  We propose a no horizon black hole whose collapsing matter condenses close to
the event horizon and before its formation. Compared to Vaz's model [arXiv:
1407.3823], our interior geometry depends only on one parameter $r_{0}$ - the
radius of the region where quantum fluctuations are significant. While the
equation of state of the inner fluid is $p_{r} = -\rho$ and the traverse
pressures are vanishing, the surface stress tensor corresponds to an
anisotropic fluid with negative surface tension. Using the junction conditions
on the boundary of the collapsing star, we found that $r_{0}$ is half its
Schwarzschild radius and not $2M$, as previously obtained by Vaz for a dust
ball.
