The galaxy appears to be a single, relatively smooth object. Its overall shape is elliptical, exhibiting a high degree of circular symmetry. There are no discernible spiral arms or a distinct disk structure. The light is centrally concentrated, with a bright core that gradually fades towards the outer edges. The color profile seems to be relatively uniform across the galaxy, with hints of bluer hues, potentially indicating ongoing, albeit moderate, star formation. There is no visual evidence of any major ongoing merging events or significant tidal disturbances. Some minor asymmetry or disturbance cannot be completely ruled out at this resolution, as the light appears slightly unevenly distributed.
