This galaxy appears to be a relatively smooth, elliptical-type galaxy. The core exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population and diminished star formation within the central region. Moving outward from the core, the galaxy's color gradually transitions to a more diffuse, greenish-blue halo, indicative of the presence of some younger stars or ongoing, though subdued, star formation in the outer regions. The morphology is largely undisturbed, lacking prominent tidal features or signs of recent major mergers, though there may be a minor gravitational interaction occurring. The galaxy possesses a roughly rounded shape, with only a slight elongation visible along one axis. Overall, this galaxy seems to be a massive, evolved system, experiencing a low rate of star formation.
