The galaxy appears as a slightly elongated, elliptical structure with a smooth, diffuse light distribution, indicating an evolved stellar population. It has a subtle color gradient, appearing more yellowish towards the center, suggesting older stars are concentrated there. The outer regions are slightly bluer, possibly due to recent star formation. No prominent spiral arms or bar structures are discernible. The overall morphology suggests it could be an elliptical galaxy, or potentially a lenticular galaxy seen at an oblique angle. There are no indications of any major ongoing merger activity. The color is largely homogenous which could be caused by internal dust obscuration or simply uniform stellar ages in most areas.
