The galaxy appears as a centrally concentrated object with a smooth morphology. It exhibits a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars. The light distribution is concentrated towards the center, fading gradually towards the edges. There is little evidence of spiral arms or distinct features, and no indications of active star formation regions. The overall structure appears relatively undisturbed, with no signs of ongoing or recent major mergers. The galaxy has an elliptical shape and is moderately sized, appearing to be a mature system with minimal recent star formation activity.
