The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness and radial symmetry in its overall light distribution. The central region shows a bright, concentrated core, suggesting a significant density of stars. There is a subtle color gradient observed, transitioning from a yellow-white core outwards to a slightly bluer halo. While the primary structure appears undisturbed, closer inspection reveals a potential faint tidal feature extending outward, possibly indicative of a minor past interaction. The overall appearance indicates a substantial stellar mass. There is evidence of some recent or ongoing star formation, although it is relatively modest. The galaxy is not currently undergoing a major merger event.
