The observed galaxy presents as a somewhat flattened elliptical shape, with a smooth, diffuse light distribution that exhibits a centrally concentrated structure. The light is noticeably more intense at the core, fading gradually outwards to an indefinite boundary. There is a slight asymmetry or perturbation visible in the outer regions, potentially indicative of minor gravitational interactions or past merger events. The galaxy appears to be mostly smooth, but has a slight disk feature that is difficult to resolve due to the resolution of the image. There is a possibility that the system is undergoing a minor disturbance. The galaxy is neither perfectly round nor significantly elongated. It appears more ovoid. The color profile suggests dominant emission in the green part of the spectrum.
