The galaxy presents as a relatively smooth, centrally concentrated object with a near-circular morphology. The light profile suggests minimal disk-like features or spiral arms. The primary color is a yellowish-orange hue, indicative of a stellar population dominated by older, less massive stars, with a low ongoing star formation rate. There is no strong indication of significant dust lanes or obscured regions within the galaxy. The overall appearance is consistent with that of an elliptical galaxy at moderate redshift. Close inspection does not reveal signs of significant tidal disturbances or ongoing mergers.
