The galaxy appears to be a relatively compact system, generally elliptical in shape, with a smooth, diffuse light distribution. The color gradient suggests a centrally concentrated population of stars. The central region exhibits a bright, blue hue which could indicate the presence of some ongoing star formation, although the system as a whole lacks prominent spiral arms or other features associated with intense star formation. There are no obvious signs of tidal disturbances or major mergers. The galaxy appears largely undisturbed.
