NGC 7625. - The bright central part of this galaxy has been studied by Lynds and Furenlid (1973). The observational data were based on the photographs shown in this catalog and photograph colors and magnitudes were obtained. Several discrete HII regions were identified and evidence was given for the existence of interstellar reddening in the dust lanes. The central 4" of the nucleus appears to have a continuum which is redder than the surrounding region.