The galaxy exhibits a smooth, elliptical morphology. Its light profile appears centrally concentrated with a distinct nucleus. A gradual decrease in luminosity emanates outwards from this core. There is no apparent spiral structure, dust lanes, or other features typically associated with disk galaxies, suggesting it is most likely an elliptical galaxy. The galaxy is yellowish/reddish in color suggesting an older stellar population. There is no evidence of any recent or ongoing major merger activity. The galaxy has a moderate redshift, indicating that it is a fairly distant object, and a high mass.
