The galaxy appears as a relatively smooth, centrally concentrated object. Its color profile indicates a redder, more evolved stellar population, particularly within the central bulge region, which emits strongly. The outer regions show hints of bluer hues, potentially indicating some ongoing, though subdued, star formation. The overall morphology is consistent with an elliptical galaxy or a lenticular galaxy viewed face-on. There is no obvious spiral structure or significant dust lane obscuration visible in this image. The galaxy's shape appears roughly circular, with no pronounced elongation or asymmetry detected. Any merging events or tidal disturbances appear to be minimal or absent.
