Relatively low q < 1.90 and unresolved (<1 arcsec) radio source (White
et al. 1997) suggest the radio source is powered by an AGN.
In close pair (Kara 147) with NGC 2474.
Close pair with NGC 2474.
HMS Note No. 039
Slit on both members of close pair NGC 2474 - NGC2475.
Weak exposure with clouds shows only spectrum of brightest
component in measurable strength.