The object presents as a single, relatively smooth and rounded galaxy. Its light profile suggests a concentrated central bulge surrounded by a less dense halo or disk. The color appears to be predominantly yellow-red, indicating an older stellar population and/or significant dust obscuration. There is no obvious spiral structure or irregular features, nor is there evidence of a major ongoing merger. A slight asymmetry is visible, potentially indicating a minor disturbance or interaction with a smaller companion object. The overall appearance is consistent with an elliptical galaxy at a moderate redshift, and the lack of prominent blue regions suggests a low star formation rate.
