The galaxy presents a generally smooth, elliptical morphology. Its light distribution exhibits a centrally concentrated bulge with a gradual decrease in intensity towards the outer regions. The galaxy core appears yellowish, suggesting an older stellar population. There's little evidence of prominent spiral arm structures or significant dust lanes. The isophotes appear mostly regular, indicating a lack of major ongoing mergers or tidal disruptions, although there may be some minor disturbances in the outer envelope of the galaxy. The size of the galaxy is relatively moderate, with the overall appearance consistent with an elliptical galaxy at a considerable distance, as indicated by its redshift.
