The galaxy presents as a single, relatively smooth and concentrated light source. It exhibits a generally elliptical morphology, appearing nearly circular. The light is concentrated towards the center, with a gradual decrease in intensity outwards. There is no discernable spiral arm structure, bar, or clear evidence of tidal disturbances or ongoing mergers. Color gradients across the galaxy are subtle, but suggest a slightly bluer central region transitioning to redder outskirts. This could indicate the presence of younger, hotter stars in the central region and a more dominant population of older, cooler stars in the outer regions.
