This galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a morphology somewhere between elliptical and lenticular, though a slight disk-like structure may be present, hinting at a possible spiral component viewed at a shallow inclination. There is some asymmetry in the light distribution, with a slight extension or tidal feature visible on one side, indicating a possible past interaction or merger event. The central region appears bright and yellowish-white, which could be indicative of a population of older stars, while fainter, slightly bluer hues on the outskirts are perhaps suggestive of younger stellar populations and ongoing, but possibly low, levels of star formation. The object appears to be reasonably massive.
