The galaxy appears to be an elliptical galaxy exhibiting a smooth, concentrated morphology. The central region displays a bright, yellowish-white hue, suggestive of an older stellar population. The galaxy exhibits a slight elongation, appearing more oblate than perfectly spherical. There is a subtle colour gradient, with the outer regions displaying a hint of green, possibly indicative of some ongoing, but limited, star formation, or perhaps influenced by the redshift of the object. No distinct spiral arms or dust lanes are visible. The overall appearance is that of a relatively undisturbed system. There is no strong evidence of a major ongoing merger, though there may be a minor tidal disturbance based on the irregularity of the green color in the outer regions.
