The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. Its overall morphology suggests a classification leaning towards elliptical or lenticular, with minimal discernible disk features. There may be a very slight asymmetry, but it does not appear to be severely disturbed by any ongoing major mergers.

The galaxy displays a color gradient, appearing bluer in the central regions and gradually becoming redder towards the outskirts. This suggests a higher concentration of younger, hotter stars in the core, with an aging stellar population further away from the center. The size is relatively compact and consistent with other similar sized galaxies in the distant universe.
