The galaxy presents as a relatively smooth, elliptical or lenticular structure. There is a distinct central bulge, appearing yellowish-white, that dominates the galaxy's light output. The outer regions appear more diffuse, fading into the background with a slightly bluer hue compared to the core. There's little evidence of spiral arms or significant dust lanes. The overall morphology suggests a system that has undergone significant evolution, potentially involving a decline in active star formation. The structure is largely undisturbed, with only a few signs of minor tidal features, implying relative isolation in its environment or a previous minor merger event.
