The galaxy presents an elliptical morphology, appearing as a generally smooth, centrally concentrated structure. Its core region exhibits a yellow-orange hue, suggesting a population of older, redder stars. Fainter, greenish-blue extensions are observed surrounding the central bulge. The galaxy appears relatively undisturbed. It exhibits a slight deviation from perfect circularity, but does not display any pronounced tidal features or signs of a major ongoing merger event. The overall color profile indicates a relatively low current star formation rate.
