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New high-resolution r band imaging of the brightest cluster galaxy (BCG) inAbell 85 (Holm 15A) was obtained using the Gemini Multi Object Spectrograph.These data were taken with the aim of deriving an accurate surface brightnessprofile of the BCG of Abell 85, in particular its central region. The newGemini data show clear evidence of a previously unreported nuclear emissionthat is evident as a distinct light excess in the central kiloparsec of thesurface brightness profile. We find that the light profile is never flat nordoes it present a downward trend towards the center of the galaxy. That is, thenew Gemini data show a different physical reality from the featureless,"evacuated core" recently claimed for the Abell 85 BCG. After trying differentmodels, we find that the surface brightness profile of the BCG of Abell 85 isbest fit by a double Sersic model.

The Abell 85 BCG: a nucleated, core-less galaxy