The galaxy presents an elliptical morphology, appearing largely featureless and smooth in structure. It exhibits a concentrated central bulge that gradually diffuses outward into a less defined halo. Color gradients are subtle; the core displays a slightly bluer hue, possibly indicating a small amount of recent star formation, while the outer regions tend towards redder tones, which suggest an older stellar population. The overall shape is somewhat elongated. There is no sign of a spiral arm structure or significant dust lane.
