The galaxy presents a largely smooth morphology, exhibiting a high degree of radial symmetry. Its color is dominated by yellowish hues in the central region, transitioning to greenish tones further outwards, suggesting a possible radial gradient in stellar populations or dust content. The light distribution indicates a relatively concentrated core, surrounded by a more diffuse halo. There is no visual evidence of strong spiral arms or a prominent disk structure. The galaxy appears generally undisturbed with no major mergers or tidal features detected.
