The galaxy presents as a relatively smooth, elliptical-like object. The light profile appears concentrated towards the center, with a gradual decrease in brightness outwards. There is a subtle elongation, but overall it exhibits a generally rounded morphology. The core region displays a distinct yellowish-orange hue, suggesting an older stellar population and minimal ongoing star formation. A bluer region is present closer to the core, indicating some degree of recent star formation in the central regions. No prominent spiral arms or distinct dust lanes are discernible. Minor disturbances are possibly present. The galaxy shows no strong signs of a major ongoing merger, though there could be an interaction or minor merger occurring. The light appears slightly redder, indicating that it is most likely located at a high distance.
