The galaxy appears as a yellowish-white, relatively smooth object. Its morphology is generally elliptical or spheroidal, with minimal discernible disk-like features or spiral arms. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity outwards from the core. There is a slight elongation in the shape of the galaxy. There appears to be no significant dust lane obscuring the core, nor any substantial tidal disturbances or ongoing mergers visible in this image. The overall appearance suggests a galaxy composed primarily of older stellar populations, lacking extensive current star formation.
