The galaxy presents a generally smooth appearance, with no immediately discernible spiral arms or bar structure. The light distribution suggests a centrally concentrated mass. The color of the galaxy appears to be yellowish-orange, implying a relatively older stellar population and reduced ongoing star formation. The overall shape of the galaxy is somewhat elliptical. There is a possibility of a minor disturbance or interaction as the galaxy has a slightly irregular appearance, indicating potential tidal features or ongoing merger activity.
