The galaxy appears to be a relatively smooth, elliptical system. The light profile suggests a high degree of central concentration. It possesses a yellowish hue. There are no obvious spiral arm structures or dust lanes visible, which reinforces the classification as an elliptical. No signs of major mergers are observed, though minor disturbances cannot be entirely ruled out. The overall roundness of the galaxy is notable, with a slight deviation from perfect circularity being potentially present.
