  We study a novel phenomena of smearing of black hole horizons from the effect
of space noncommutativity. We present an explicit example in $AdS_3$ space,
using the Chern-Simons formulation of gravity. This produces a smeared BTZ
black hole which goes beyond the classical spacetime unexpectedly and there is
{\it no} reality problem in our approach with the gauge group $U(1,1) \times
U(1,1)$. The horizons are smeared, due to a splitting of the Killing horizon
and the apparent horizon, and there is a metric signature change to Euclidean
in the smeared region. The inner boundary of the smeared region acts as a
trapped surface for timelike particles but the outer as a classical barrier for
ingoing particles. The lightlike signals can escape from or reach the smeared
region in a {\it finite} time, which indicates that {\it the black hole is not
so dark, even classically.} In addition, it is remarked that the Hawking
temperature can {\it not} be defined by the regularity in the Euclidean
geometry except in the non-rotating case, and the origin can be smeared by a
{\it new} (apparent) horizon.
