The galaxy presents as a roughly circular, smooth, and concentrated spheroid of light. It exhibits a distinct central bulge that is intensely luminous, suggesting a high density of stars and possibly a supermassive black hole actively accreting matter at its core. The color appears yellowish, which could indicate a population of older, cooler stars dominating the light output. There is no apparent spiral arm structure or significant dust lane obscuration. The overall morphology suggests an elliptical galaxy type, potentially a massive one, with no immediately obvious signs of ongoing major mergers or tidal disturbances. The light is distributed relatively evenly, lacking prominent substructure or distinct star-forming regions. The apparent size is small, consistent with its considerable distance.
