The galaxy presents as a fairly smooth, elliptical-like structure with a dominant central bulge. The object appears largely featureless, lacking prominent spiral arms or distinct dust lanes. Its color is generally yellow, suggesting an older stellar population with fewer young, hot stars. There is potentially a hint of a disk component, but it is not clearly defined. Based on the roundness of the galaxy and the smoothness of the image, it is possible there is ongoing or recent merging activity, with only minor signs of disturbance or tidal features.