The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated core that gradually diffuses outward into a more extended, fainter halo. The overall color appears to be dominated by older stellar populations, with a yellowish hue. The shape is somewhat elongated, suggesting a possible transition between a spherical and more flattened elliptical form. There is no obvious presence of spiral arms or significant dust lanes. Minor irregularities or disturbances are visible, suggesting a potential minor interaction or past merger event.
