The galaxy presents as a relatively smooth, elliptical-like object. It appears largely featureless, lacking prominent spiral arms or distinct substructures. The galaxy exhibits a concentrated central bulge. There may be two distinct components that are in the process of merging into a larger elliptical galaxy. The color profile leans towards the redder end of the spectrum, suggesting an older stellar population and low dust content. There is only a small amount of star formation activity and the size of the galaxy is a few kiloparsecs across.
