The galaxy presents a generally smooth and elliptical morphology. Its core is characterized by a concentrated region of yellow-white light, suggesting a significant population of older stars. The outer regions display a gradual decline in luminosity, exhibiting a diffuse and less structured appearance. There are no apparent spiral arms or significant dust lanes visible in this image. The galaxy's overall color profile indicates a population dominated by older stars, hinting at a low rate of ongoing star formation. Slight color variations are visible within the galaxy's halo, possibly indicating subtle changes in stellar populations across different radii. There is a slight asymmetry present, hinting at a potential past interaction or merger.
