The galaxy exhibits a generally smooth morphology, appearing elliptical or lenticular upon visual inspection. There is a central concentration of light, suggesting a prominent galactic nucleus. The overall shape is relatively round. A slight color gradient is observable, shifting from a reddish hue in the core to a bluer tint in the outer regions. This could indicate older stellar populations concentrated in the center and younger stars present in the outer portions of the galaxy. No distinct spiral arms or significant dust lanes are apparent. The galaxy appears relatively undisturbed, with no indications of ongoing major mergers or tidal interactions. The galaxy is consistent with being a relatively massive system, exhibiting moderate star formation.
