ABSTRACT
Crossley reflector photographs show that Caswell's identification for the optical associated with the compact radio source centered on B127.11+0.54 is indeed a luminous obscured galaxy, similar to M87. IDS spectra show emission lines of [N II], Hα, and [S II] (in order of strength) in the red, yielding a heliocentric radial velocity of +5490 ± 90 km s-1. Our velocity and conclusions as to the extragalactic nature of the central source are in good agreement with those of Kirshner and Chevalier.