The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits high luminosity, appearing nearly spherical with a concentrated core. A slight flattening is observed from the core outwards, transitioning to a more lenticular shape along the major axis. There appears to be some degree of distortion, possibly indicating an interaction. Color gradients suggest a slightly bluer spectral energy distribution in the outer regions compared to the core, implying a somewhat larger presence of younger stars away from the center of the galaxy. No distinct spiral arm structures are discernable. The size of the galaxy appears moderate.
