The galaxy presents as an elliptical morphology, appearing mostly smooth with little discernible internal structure. The light profile appears centrally concentrated with a gradual decrease in luminosity outwards, suggesting a substantial bulge component. The color gradient shifts from a yellow-white core to a bluer outer halo, indicating the presence of older stellar populations in the center and relatively younger populations in the outer regions. There may be faint indications of tidal features or minor disturbances, though these are not prominent and could be due to image artifacts or the superposition of background objects. The overall impression is of a relatively evolved galaxy, undergoing low levels of star formation activity if any.
