The galaxy presents an elliptical morphology, with a high degree of central concentration. It exhibits a smooth, featureless appearance. There is a lack of discernible spiral arms or a prominent disk structure. The galaxy appears approximately round, with a slight deviation from perfect circularity. There is no obvious indication of any major ongoing merger events or significant tidal disturbances. Color gradients suggest the presence of an older stellar population, with a possible slight decrease in star formation activity, and a relatively high mass.
