The galaxy presents as a fairly smooth, centrally concentrated object. It displays a notable elliptical morphology, with an approximate axis ratio of close to 1:1 indicating it is mostly round. There are no obvious spiral arms or a prominent disk structure visible at this resolution. The galaxy appears largely undisturbed, showing no major signs of ongoing mergers or significant tidal disturbances. Its core region exhibits a slightly more concentrated brightness, potentially indicative of an active galactic nucleus or a higher density of stars in the central bulge. The observed color suggests a dominant population of older stars, as the overall color is more consistent with light emitted from redder stars, although there is some suggestion of star formation in the bluer parts of the galaxy. Overall, the galaxy appears to be a moderately massive elliptical galaxy at a considerable distance.
