The galaxy presents as a single, centrally concentrated object. The light distribution is smooth, lacking distinct spiral arms or a prominent disk structure. The overall shape appears largely round. There is some evidence of minor disturbance within the system, visible as a slight asymmetry. The object displays a color gradient, appearing more red in the central regions and with less intense blue outer regions. The lack of a strong blue color suggests the galaxy may be largely composed of older stellar populations and minimal current star formation. There may be interaction or merger events occurring, and a deeper investigation may be warranted.
