The galaxy presents as a relatively compact elliptical structure, with a smooth, centrally concentrated light profile. A slight elongation is visible, suggesting a degree of flattening or asphericity. The color appears to be generally yellow-white in the central region, indicative of an older stellar population. A subtle gradient towards bluer hues is observed in the outer regions, possibly indicating the presence of younger stars, or a recent minor merger. There are no distinct spiral arms or dust lanes visible in this image. Any present star formation would likely be occurring at a relatively low rate. The overall structure seems undisturbed, suggesting a lack of major recent interactions.
