The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a concentrated brightness, indicating a possible bulge component. The color gradient transitions from a redder core to a slightly bluer outer halo, suggesting variations in stellar populations or dust content. No distinct spiral arms or bar structures are discernible. The overall shape approximates an ellipse, with a moderate ellipticity, appearing slightly elongated. There are no apparent signs of major mergers or significant tidal disturbances. The galaxy appears relatively undisturbed and quiescent. The inferred stellar mass is substantial, corresponding to a large galaxy. The star formation rate is estimated to be low.
