The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge, with a gradual decrease in luminosity outwards. The galaxy's color profile suggests an older stellar population. The core of the galaxy shows a yellow hue, while the outer regions appear redder. There is little to no evidence of spiral arm structures or significant dust lanes. Minor irregularities or disturbances in the galaxy's shape cannot be ruled out, but it appears to be a fairly relaxed system. There is no obvious sign of ongoing major merging events, though the possibility of minor interactions cannot be excluded based on this single image. The object has a round overall shape.