The galaxy presents as a relatively smooth, elliptical structure. Its overall color profile suggests a dominant population of older stars, exhibiting a yellowish-orange hue concentrated toward the central bulge. The shape is slightly elongated, appearing more lenticular than perfectly spherical. There are no prominent spiral arms visible, and the smoothness of the light distribution indicates a lack of significant recent star formation activity. Minor disturbances, such as tidal tails or asymmetric features, are not apparent upon visual inspection of this image, suggesting that the galaxy is not currently undergoing a major merger event.
