The galaxy appears as a centrally concentrated, generally smooth object. There is a slight elongation, but overall it is close to circular in projection. The light profile suggests a bulge-dominated system. The central region is bright and transitions smoothly to fainter outer regions. There is a suggestion of color variation, with a slightly redder central core and bluer outer regions. There is no evidence of spiral arms, bars, or other distinct features. It is likely a fairly massive galaxy with moderate star formation activity. There is no evidence of significant tidal disturbances or ongoing mergers.
