The galaxy presents as a largely featureless elliptical structure. The central bulge exhibits a strong concentration of light, appearing a yellow-orange hue, likely indicating an older stellar population. Moving outward from the core, the light gradually diffuses into a more extended halo. The outer regions show a subtle transition to a slightly bluer tint. The overall shape deviates slightly from a perfect circle, presenting a mild elongation along one axis and a relatively smooth texture. There is no apparent evidence of spiral arms or significant dust lanes. Subtle disturbances or minor asymmetries may be present.
