The galaxy presents as a somewhat elliptical, centrally concentrated object with a diffuse halo. The central region is bright and appears yellowish-white in color, suggesting an older stellar population. The overall structure seems relatively smooth, with only subtle indications of any spiral arm features or distinct substructures. There is a slight elongation along one axis, lending it a flattened appearance. The halo extending beyond the core is fainter and appears slightly bluer, possibly indicating a younger population of stars at the periphery or ongoing star formation, though this could also be influenced by redshift effects. There is a possible faint tidal feature on one side, suggesting the possibility of a past interaction or merger event.
