The galaxy presents a relatively smooth, elliptical morphology. It exhibits a centrally concentrated bulge region that fades gradually outwards to a more diffuse halo. The light distribution suggests a relatively well-mixed stellar population throughout, with minimal evidence of distinct spiral arm structures or significant dust lanes. Subtle color variations are present, showing a slightly bluer hue in the outer regions, indicative of ongoing, though likely low, levels of star formation. Overall, the galaxy appears largely undisturbed, with a slight chance of minor merger.
