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We model the spectral energy distribution of the ultrasoft broad-line AGN REJ2248-511 with Comptonised accretion disc models. These are able to reproducethe steep optical and ultrasoft X-ray slopes, and the derived black hole massis consistent with independent mass estimates. This AGN displays properties ofboth broad and narrow line Seyfert 1 galaxies, but we conclude that it isintrinsically a `normal' Seyfert 1 viewed at high inclination angle.Comment: 4 pages, 1 figure. MG10 Proceeding

THE SOFT X-RAY EXCESS AGN RE J2248-511