NGC 4192 (UGC 7231, 1211+1510)

NGC 4192 (UGC 7231, 1211+1510) -- This highly-inclined Sb galaxy has a nucleus with strong optical emission lines, with line ratios intermediate between a LINER and an H II nucleus, and indicative of reddening (Ho et al. 1996a). Its UV image shows three amorphous knots of very weak emission.