The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. It exhibits a color gradient, transitioning from a yellowish core region outwards to a bluer halo. The smoothness and roundness suggest that the galaxy is unlikely to be undergoing major mergers and the lack of defined spiral arms further supports this hypothesis. There's a slight asymmetry in the outer regions, with some possible faint tidal features present, but they are relatively subtle. Overall, the galaxy appears as a relatively evolved system with ongoing but not excessively high star formation.
