This galaxy appears as a centrally concentrated object, exhibiting a primarily smooth morphology. Its overall shape is somewhere between round and elliptical, with a slight elongation noticeable. The galaxy's core is bright and compact, suggesting a significant concentration of older stellar populations. The lack of prominent spiral arms or dust lanes indicates a relatively undisturbed structure. Faint, diffuse light extends outwards from the core, creating a halo-like structure surrounding the galaxy. There are no obvious signs of recent major mergers, but a minor disturbance cannot be entirely ruled out. In summary, the galaxy presents as a relatively evolved, quiescent system, consistent with an elliptical or S0 classification.
