The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a noticeable decrease in light intensity from the center outwards. The core region is bright, with an off-white hue, suggestive of an older stellar population. Surrounding the core, a more diffuse, blue-green halo is visible. This could potentially indicate the presence of some ongoing, albeit low, levels of star formation, or perhaps a population of older, hotter stars. The lack of prominent spiral arms or significant dust lanes further supports the classification of this galaxy as an early-type galaxy. The overall structure appears relatively undisturbed, showing no signs of major mergers or interactions. However, there are subtle features that may be indicative of a minor disturbance or past interaction, although it is difficult to ascertain their origin with certainty from the image.
