The galaxy presents as an elliptical morphology with a smooth, centralized light distribution. The core exhibits a bright, concentrated region, suggestive of a high stellar density. The color profile indicates a yellowish hue in the central region, possibly indicating an older stellar population. The outskirts appear slightly bluer, which could be due to ongoing, albeit limited, star formation. There are no clear spiral arm structures visible, and the galaxy appears relatively undisturbed, exhibiting no signs of major mergers or significant tidal interactions. There might be a very slight dust lane or other feature causing the galaxy to appear slightly elongated, but this is uncertain given the image resolution.
