  Sensitive radio continuum surveys of the Galactic plane are ideal for
discovering new supernova remnants (SNRs). From the Sino-German {\lambda}6 cm
polarisation survey of the Galactic plane, an extended shell-like structure has
been found at l = 21.8 degree, b = -3.0 degree, which has a size of about 1
degree. New observations were made with the Effelsberg 100-m radio telescope at
{\lambda}11 cm to estimate the source spectrum together with the Urumqi
{\lambda}6 cm and the Effelsberg {\lambda}21 cm data. The spectral index of
G21.8-3.0 was found to be {\alpha} = -0.72 {\pm} 0.16. Polarised emission was
mostly detected in the eastern half of G21.8-3.0 at both {\lambda}6 cm and
{\lambda}11 cm. These properties, together with the H{\alpha} filament along
its northern periphery and the lack of infrared emission, indicate that the
emission is non-thermal as is usual in shell-type SNRs.
