  We discuss the optical spectrum of a multiply-imaged arc resolved by HST in
the $z$=0.175 cluster A2218. The spectrum, obtained with LDSS-2 on the 4.2m
William Herschel telescope, reveals the source to be a galaxy at a redshift
$z$=2.515 in excellent agreement with the value predicted by Kneib et al.
(1996) on the basis of their inversion of a highly-constrained mass model for
the lensing cluster. The source is extremely blue in its optical-infrared
colours, consistent with active star formation, and the spectrum reveals
absorption lines characteristic of a young stellar population. Of particular
significance is the absence of Lyman-$\alpha$ emission but the presence of a
broad Lyman-$\alpha$ absorption. The spectrum is similar to that of other, much
fainter, galaxies found at high redshift by various techniques and illustrates
the important role that lensing can play in detailed studies of the properties
of distant galaxies.
