The galaxy presents as a relatively smooth and centrally concentrated object. Its overall shape is elliptical, appearing somewhat rounded but with a slight elongation. The central region exhibits a bright, yellowish hue, indicative of a high concentration of older stellar populations. Surrounding the core, there's a more diffuse, fainter halo or disk-like structure. There are hints of blueish regions within the disk, suggesting the presence of some younger stars. No obvious spiral arm structures or major disturbances are apparent. The overall color gradient suggests a transition from older stars in the core to a mix of stellar populations in the outer regions. The morphology indicates it is likely a massive galaxy with a low star formation rate.
