The galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a bright, yellowish-white core, indicative of a high concentration of older stars. The light appears to gradually fade from the core outwards. The outer regions show a slight bluer hue, possibly indicating the presence of younger stars or ongoing, albeit minimal, star formation. There are no clear spiral arms, bar structures, or significant dust lanes visible in this image. The galaxy’s overall form presents a smooth, rounded shape with no signs of significant merging activity or major disturbances.
