The galaxy appears as a single, centrally concentrated object. It exhibits an elliptical morphology with a smooth light distribution, suggesting a relatively old stellar population. The color appears to be somewhat redder, possibly indicating the presence of a more evolved stellar population with lower rates of star formation. There are no clearly discernible spiral arms or bar features. Based on the color, the galaxy appears to have a red shift indicating it is a distant object. No apparent signs of recent or ongoing major merger events are observed; however, subtle disturbances may be present.
