Merging double galaxy; both components appear to contribute to the
NVSS and FSC sources.
NGC 7250; S/I, starburst.
This galaxy appears as a interacting double system (Markaryan et al.
1985). The presence of absorption lines typical of hot stars suggests
that NGC 7250 has active star formation. However, it is difficult to
distinguish absorption features due to the galaxy itself from those of
the Milky Way. In addition, the IUE camera artifacts are evident here.
Probably a companion superimposed at 0.4, 335, 0.25 x 0.18
NGC 7248 is at 17.5 arcmin.