The object presents as a single, relatively smooth galaxy. It exhibits a flattened, elliptical morphology. The central region appears brighter and more concentrated, showing a yellowish-orange hue, suggestive of an older stellar population. Extending outward from the core is a fainter, more diffuse halo. This outer region transitions in color to a slightly bluer tone, possibly indicating the presence of some younger stars or ongoing star formation. There are no prominent spiral arms or bar structures readily apparent in this image, and the overall appearance suggests a system that has largely settled into a more quiescent state. There is a hint of a minor disturbance in the outer regions.
