The galaxy presents an elliptical morphology, appearing somewhat elongated with a major axis likely exceeding its minor axis by a noticeable amount. Its overall color profile appears yellowish-white, hinting at a stellar population dominated by older, evolved stars. The light distribution seems relatively smooth, suggesting that the galaxy has undergone significant dynamical relaxation. Evidence of spiral arms or prominent dust lanes is not apparent. Faint, reddish tinges are visible toward the periphery, which could indicate the presence of older red giant stars or the existence of some residual star formation, albeit at a low rate. No substantial tidal features or other signatures of recent or ongoing mergers are readily discernible in this image. The galaxy shows no clear signs of a distinct central bulge or a pronounced disk component.
