The galaxy appears as a centrally concentrated, somewhat elliptical structure with a yellowish hue. It exhibits a smooth light profile, with no prominent spiral arms or distinct features readily apparent. The galaxy appears relatively round. There are suggestions of redder, less intense light, primarily at the core and fading as we reach the edges. The lack of distinct features might indicate that it is a galaxy with little current star formation, and is comprised of old stars. No obvious merger activity is observed.
