The galaxy exhibits a morphology consistent with an elliptical galaxy. It presents as a smooth, centrally concentrated luminosity profile, with no discernible spiral arms or significant dust lanes. The overall shape is elongated, suggesting a moderate degree of ellipticity. The central region is a bright yellow, while the outer regions appear redder, indicating a potentially older stellar population. The light is relatively uniform, with no distinct clumps or regions of intense star formation readily apparent. There are no obvious signs of tidal disturbances or ongoing mergers; it is a relatively undisturbed, evolved system.
