The galaxy presents a generally smooth, elliptical morphology. It exhibits a central bulge that appears yellowish-orange, indicative of an older stellar population. The isophotes suggest the galaxy is somewhat elongated, deviating from a perfectly spherical shape. The outer regions display a fainter, bluer hue compared to the core. There is a faint suggestion of a disk component, or other larger feature, but overall it looks like an elliptical galaxy with no signs of major disturbances or ongoing merger activity.
