The galaxy presents a primarily smooth morphology, with a dominant spheroidal component. The light distribution appears highly concentrated towards the center. There is a subtle elongation or ellipticity to the overall shape. Color gradients suggest the presence of older stellar populations in the central regions, which appear more yellow/red, while the outer regions are slightly bluer, potentially indicating the presence of younger stars. There are no visually discernible spiral arms or significant dust lanes. No indications of major merger events or strong tidal disturbances are apparent. Based on its visual characteristics, the galaxy is potentially an elliptical or an S0 type.
