The observed galaxy presents a primarily smooth morphology with a slightly irregular shape. The object displays a bright central core region. There is a hint of extended structure, possibly a faint disk component or tidal feature, surrounding the core. The overall color profile indicates the likely presence of a mix of stellar populations, with a notable blue component potentially suggesting ongoing or recent star formation, superimposed on a more dominant population of older stars. Faint disturbances are present, suggestive of possible minor interactions or recent mergers.
