  Redshifts of several galaxies thought to be associated with NGC 326 are
determined. The results confirm the presence of a cluster and find a mean
redshift of z = 0.0477 +/- 0.0007 and a line-of-sight velocity dispersion
sigma_{z} = 599 (+230, -110) km/s. The velocity dispersion and previously
measured X-ray gas temperature of kT ~ 1.9 keV are consistent with the cluster
sigma_{z}/kT relation, and NGC 326 is seen to be a slowly-moving member of the
cluster.
