NGC 424
NGC 424 is a spiral galaxy in the constellation of Sculptor. Its velocity with respect to the cosmic microwave background is, which corresponds to a Hubble distance of. Also, two non-redshift measurements give a similar mean distance of. It was discovered by British astronomer John Herschel on November 30, 1837.
NGC424 is a Seyfert I 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.