  We report the discovery of a new SNR in the \ros All-Sky-Survey data. The SNR
has a nearly circular shape with a diameter of about 15 arcmin. The surface
brightness is rather uniform over the remnant. The observed interstellar
absorption suggests a distance of about 1.8$^{+1.4}_{-0.8}$ kpc. The X-ray
emission appears to be of thermal origin with a plasma temperature of about
10$^7$ K. The Sedov model leads to an age of only 1800 years. We find no
spectral evidence of non-thermal emission in the center of the remnant. The two
most likely explanations for the centrally filled structure are evaporation of
shock heated clouds in the interior of the remnant or a reverse shock heating
the ejecta of the SNR explosion.
