The galaxy presents as a centrally concentrated spheroid, exhibiting a smooth, relatively featureless morphology. It displays a yellowish-white color, suggesting an older stellar population dominating its composition. The galaxy appears to be somewhat elliptical, with a deviation from perfect circularity. There is no apparent evidence of spiral arms, a bar structure, or significant dust lanes. Furthermore, no obvious signs of ongoing or recent major merger events are discernible; the galaxy appears largely undisturbed. The radial light profile suggests a gradual decline in intensity from the core outward, lacking any distinct breaks or rings.
