The galaxy appears to be a relatively smooth, elliptical galaxy. It presents a centrally concentrated brightness profile, with the luminosity decreasing gradually outward from the core. The galaxy exhibits a generally rounded shape, with no obvious signs of strong tidal disturbances or major asymmetries. There is little evidence of distinct spiral arms or a prominent disk structure. A hint of a slight color gradient can be observed, with the central region appearing somewhat brighter and perhaps slightly redder, indicating a possible concentration of older stellar populations. The outer regions seem marginally bluer. Based on the overall morphology, this galaxy is likely undergoing only minimal current star formation activity.
