The galaxy appears as a relatively smooth, elliptical-shaped object. Its core exhibits a concentrated, bright yellowish-white light, indicating a potential accumulation of older stellar populations and potentially a supermassive black hole actively accreting matter. The light gradually fades from the center to the outer edges, with the faint outer regions appearing more reddish. There's no visible spiral arm structure or significant dust lane features within the image, suggesting that it is likely an early-type galaxy with little active star formation currently taking place. The galaxy appears well-defined, with no obvious tidal disturbances or signs of ongoing mergers. The light distribution is remarkably even, indicating a well-relaxed system.
