The galaxy presents as a centrally concentrated, smooth object with a slight elongation. Its color profile exhibits a yellowish-red hue, indicative of an older stellar population. There is a lack of discernible spiral arms or significant dust lanes. The morphology suggests an elliptical galaxy or a lenticular galaxy seen at a shallow inclination. There are no obvious signs of recent merger activity or tidal disturbances. The galaxy appears relatively isolated in the field, without nearby companions. The object is likely a massive galaxy, potentially harboring a supermassive black hole at its core. It is exhibiting low star formation activity. The overall appearance suggests a galaxy which has largely completed its star formation.
