The galaxy presents as a relatively smooth, elliptical or lenticular system, exhibiting a high degree of central concentration. The core region displays a bright, yellowish hue that fades gradually towards the outer regions. There is little indication of spiral arms or complex structures within the visible light spectrum. Overall, the galaxy has a regular, rounded morphology, with no obvious signs of major disturbances or ongoing mergers with other galaxies. The apparent color suggests a relatively old stellar population, with limited ongoing star formation.