This galaxy presents as a fairly smooth, elliptical-like structure. There is little evidence of spiral arms or significant disk features. The light is concentrated towards the center, with a gradual decrease in intensity towards the edges. The color is primarily a yellow-red hue, suggesting an older stellar population with relatively low ongoing star formation. There may be a very subtle hint of tidal disruption in the form of minor irregularities or a slight asymmetry in the outer halo, but it's not obviously indicative of an ongoing merger. Overall, it appears to be a relatively undisturbed elliptical galaxy.
