The galaxy presents as an elliptical morphology, with a smooth and concentrated central bulge. The radial color gradient indicates a change in stellar population, with the central region appearing more yellow and the outer regions exhibiting a slight bluer hue. This likely suggests older stellar populations are concentrated towards the center and younger, star-forming regions or populations are further out.

The light distribution appears relatively even and symmetrical, though a minor asymmetry or perturbation can be observed to the lower right of the galaxy. The overall structure does not exhibit prominent spiral arms or a distinct disk. There may be minor disturbances or hints of tidal features present, though more data is needed.
