The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color appears to be yellowish, suggestive of an older stellar population and diminished ongoing star formation. The morphology is broadly elliptical, showing a shape that is neither perfectly round nor distinctly elongated, but falls somewhere in between. There is no obvious evidence of a pronounced disk structure, spiral arms, or recent major merger activity. Subtle indications of a minor disturbance cannot be completely ruled out, however, the galaxy appears largely undisturbed.
