The galaxy presents an elliptical morphology, appearing largely featureless and smooth in structure. Its color gradient transitions from a concentrated, yellowish-orange core to fainter, blue-tinged outer regions, suggesting an older stellar population towards the center with potential ongoing or recent star formation in the outskirts. The galaxy exhibits a moderate degree of flattening, deviating slightly from a perfectly spherical shape, with no immediately discernible signs of major disturbances or ongoing merger events. The overall luminosity profile indicates a relatively high-mass system.
