The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated central bulge. It appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The color gradient suggests a possible difference in stellar population, transitioning from a yellowish core to a bluer, fainter halo region. The galaxy exhibits a generally rounded morphology, although a slight elongation is noticeable. There are no immediately apparent signs of ongoing major mergers or significant tidal disturbances. The overall impression is that of a galaxy undergoing relatively quiescent evolution.
