The galaxy presents as a relatively smooth, elliptical-like structure. Its core region exhibits a concentrated, bright luminosity, suggesting a high density of stars and potentially a supermassive black hole actively accreting material. This central region is enveloped by a more diffuse halo or outer envelope. There is a clear color gradient, with the core appearing more yellow/orange compared to the bluer or greener outer regions. This indicates a potential difference in stellar populations, with the core possibly dominated by older, redder stars, while the outskirts exhibit a younger, bluer stellar population, or enhanced star formation activity. There's no obvious evidence of spiral arms, bars, or significant dust lanes. The morphology points towards a mature galaxy with a high degree of spherical symmetry. There is no obvious indication of major mergers or strong tidal interactions, although minor disturbances cannot be ruled out based on the image alone.
