The galaxy presents a moderately bright central bulge that transitions smoothly outward. The primary visible light emission appears to be concentrated in this central region, with a diminishing gradient towards the edges. The galaxy's shape is generally elliptical, trending toward a flattened spheroid. Some asymmetry is apparent in the outer regions, possibly indicative of minor gravitational interaction or disturbance. There may be faint features suggesting a very weak disk. A blue region in the center may indicate star formation.
