The galaxy presents as a centrally concentrated, smooth, and largely featureless structure. It exhibits a predominantly elliptical morphology, with a high degree of circularity. There is no evidence of spiral arms or a prominent disk. The color profile suggests a relatively uniform stellar population with a possible hint of a bluer, star-forming region concentrated in the core, although this is subtle. There are no obvious signs of recent or ongoing major mergers, although the potential for minor disturbances cannot be ruled out based on this image alone. The galaxy appears relatively undisturbed and quiescent in its current state.
