The galaxy presents as a moderately compact, elliptical system. It displays a smooth, centrally concentrated light profile, suggesting an older stellar population. There is little evidence of spiral arm structure. The galaxy exhibits an intermediate ellipticity, appearing somewhat elongated but not highly flattened. There are no prominent dust lanes visible in this image, implying a low level of interstellar dust. A very slight perturbation may be present, but this is not a clear merger event. The color is slightly reddish, consistent with a redshifted galaxy at a moderate distance.
