The galaxy presents as a centrally concentrated, elliptical-like system. Its core exhibits a bright, yellowish-orange hue which indicates an older stellar population. Extending outwards from the core, fainter, diffuse regions of light are visible along what appears to be a vertical axis of symmetry. These fainter regions appear more red. The light distribution suggests that this galaxy is not perfectly elliptical but elongated. There is evidence of disturbance in its shape, possibly indicating tidal interactions or a previous merger event. Overall, the galaxy appears to be a relatively quiescent system.