The galaxy presents as a primarily smooth, elliptical form. It exhibits a concentrated central region, suggesting a significant bulge component. The light profile appears largely uniform without prominent spiral arm structures. The object displays a yellow-red hue, indicative of an older stellar population and minimal ongoing star formation. The morphology is relatively undisturbed, showing no clear signs of major mergers or significant tidal distortions. The light is fairly concentrated, without a large halo. The galaxy appears to be relatively isolated. The overall color suggests a high mass. The galaxy is generally regular in shape, though it may have a minor companion galaxy that would classify it as a binary galaxy.
