NGC 5605
NGC5605 is an intermediate spiral galaxy in the constellation of Libra. Its velocity with respect to the cosmic microwave background is 3635 ± 18km/s, which corresponds to a Hubble distance of. In addition, three non redshift measurements give a farther distance of. The galaxy was discovered by German-British astronomer William Herschel on 11 May 1784.
The SIMBAD database lists NGC5605 as a Seyfert II Galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.