The galaxy presents as a slightly elongated, elliptical form with a smooth, diffuse light distribution. The central region exhibits a higher concentration of luminosity, suggesting a prominent galactic nucleus. The galaxy displays a color gradient, transitioning from a yellowish core to a faint bluish-green periphery. This color difference may indicate varying stellar populations or dust distribution within the galaxy, with older stars concentrated in the core and younger stars distributed in the outer regions. There's a hint of a flattened disk-like structure, but without any spiral arm structure. There is no obvious evidence of active galactic nuclei or recent major merger events.
