The galaxy presents as a single, relatively smooth object with no discernible spiral arms or bar structure. It appears largely elliptical in shape, with a high degree of central concentration. The core exhibits a yellowish-white hue, suggesting an older stellar population and/or significant dust obscuration. Moving outward from the core, the galaxy displays a gradient shift toward a greenish color. This color transition suggests the presence of a younger stellar population. While largely undisturbed, there's a faint, barely perceptible asymmetry suggesting a minor interaction or tidal disturbance in its recent past. The light distribution is centrally concentrated, fading gradually toward the edges, and its apparent size is small.
