The galaxy appears as a flattened, elliptical-shaped object. Its light distribution is relatively smooth and concentrated towards the center, indicating a possible high degree of spheroidal symmetry. The galaxy presents a yellowish-white hue in its central region, subtly transitioning to a bluer tint along its outer edges. This color gradient may suggest an older stellar population dominating the core, with younger, bluer stars residing in the peripheral regions. There is no discernible spiral arm structure, and the overall form suggests a later-type disk galaxy viewed nearly edge-on, or an elliptical galaxy with some residual disk-like structure. Minimal signs of recent major merging events or significant tidal disturbances are evident in the image. There may be some minor irregularity in the outer regions, but the object is largely undisturbed.
