The galaxy presents a dual morphology, with two apparent components. One component is a bright, centrally concentrated spheroid exhibiting a smooth light distribution. The other component appears as a disk seen at an oblique angle. The disk component exhibits a more diffuse, elongated structure. The overall color of both components is generally reddish, with possible subtle variations suggesting differences in stellar populations or dust content. There is no clear evidence of strong tidal features or major ongoing mergers, though some subtle irregularity might suggest minor interactions.
