The galaxy appears as a single, concentrated source of light. It presents a smooth, elliptical morphology with a high degree of central concentration. There is little indication of spiral arms or significant disk features from this view. The light distribution is relatively uniform, with a gradual decrease in brightness from the core outwards. A slight elongation is observed, but it is generally round. There's no obvious evidence of tidal disturbances or ongoing mergers. The light emitted suggests a relatively old stellar population, as the blue light is subdued, and the galaxy is slightly red. The small size indicates the object is at a considerable distance.
