The galaxy presents as a relatively compact object with a prominent central bulge. The light distribution suggests an elliptical or lenticular morphology, with a smooth, diffuse halo surrounding the brighter core. There's a subtle suggestion of a flattened disk, though the spheroidal component dominates.

Color variations are present within the galaxy. The central region exhibits a yellowish-white hue, potentially indicating a population of older, cooler stars. The outer regions of the galaxy show a faint bluish tint which may suggest pockets of younger, hotter stars.

There appears to be a slight asymmetry or disturbance in the galaxy's shape, hinting at a possible interaction or past merger event. However, the overall structure remains largely coherent.
