The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated light profile. The overall shape is elliptical, tending towards a more rounded form but lacking a distinct disk structure. The color indices suggest a relatively evolved stellar population, likely dominated by older, redder stars. There is no apparent evidence of major mergers or significant tidal disturbances, although minor irregularities cannot be completely ruled out at this resolution. The galaxy’s luminosity indicates it is a massive system with correspondingly low ongoing star formation.
