The galaxy presents as a relatively smooth, centrally concentrated light distribution. The primary structure appears elliptical, tending towards a circular morphology, with a high degree of symmetry. There is a noticeable color gradient, with the central region displaying a brighter, cyan hue, possibly indicating a population of younger, hotter stars or an active galactic nucleus. A fainter, bluish extension is visible on one side of the primary structure, suggesting either a tidal feature or a region of enhanced star formation. There are no prominent spiral arms or other disk-like features visible within the resolution of the image. The overall appearance suggests a system that may be undergoing or has undergone a merger event, resulting in a smoothing of features.
