The galaxy appears to be a relatively smooth, elliptical or lenticular type. It displays a concentrated central bulge, indicating a significant population of older stars. The galaxy exhibits a slight elongation along one axis, suggesting a degree of flattening but overall it looks more elliptical. No prominent spiral arms or distinct dust lanes are discernible. Its color suggests a lack of recent star formation; it has a slightly yellow hue. There are signs of some disturbances, but overall this galaxy appears to be relatively isolated and undisturbed.
