The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical shape. The core region presents a bright, slightly yellowish-white glow, suggesting a concentration of older stellar populations. The galaxy transitions outward into a more diffuse halo. There is no obvious presence of spiral arms or a prominent disk structure. The color gradient suggests ongoing, but relatively low, star formation activity in the outer regions, appearing slightly blue. No major signs of tidal disruption or ongoing mergers are immediately apparent, but subtle disturbances cannot be ruled out.
