The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color appears slightly reddish, indicative of an older stellar population and potentially ongoing star formation. There is a faint suggestion of a disk-like component, though the light is smoothly distributed and the galaxy appears largely spheroidal. There does not appear to be a significant central bulge or any strong spiral arm structure. There is some minor disturbance to its smoothness possibly due to an old merger. Its shape is mostly round. The galaxy appears isolated, showing no signs of major mergers or interactions with other large galaxies, though there are minor disturbances that could indicate a past merger event.
