The galaxy presents as a somewhat smooth and elliptical structure, appearing more elongated than circular. The light profile exhibits a strong central concentration, characterized by a bright, yellowish core that suggests an older stellar population. There's a gradual decrease in luminosity moving outwards from the core, with a surrounding halo that presents as a faint, diffuse bluish haze. No distinct spiral arms or bar structures are discernible. There are hints of minor disturbances but no indication of a major ongoing merger. Overall, the galaxy gives the impression of a mature, relatively undisturbed system.
