The galaxy presents a generally smooth morphology with a centrally concentrated luminosity profile. A slight elongation is discernable, but the galaxy appears largely spheroidal in shape. The core exhibits a yellowish hue, suggesting an older stellar population. The outer regions display a more diffuse and bluer color, possibly indicating some ongoing, albeit weak, star formation. There's no strong evidence of spiral arms or a defined disk structure. The image does not reveal any substantial signs of tidal disturbances or ongoing mergers, although there might be some minor asymmetries present. The overall appearance suggests an elliptical or S0 galaxy at a considerable distance.
