The galaxy appears as a somewhat elongated, though not perfectly spherical, structure. The light distribution suggests a bulge-dominated morphology, presenting a smooth light profile with no clearly resolved spiral arms. It displays a yellow-orange hue, possibly indicating an older stellar population with lower ongoing star formation within the galaxy. There is a suggestion of some minor internal structure or disturbance based on some asymmetries in the light distribution, however, the bulk of the galaxy is relatively undisturbed.
