The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse morphology. Its color profile appears reddened, especially toward the central bulge, which is likely composed of older stellar populations. There is a subtle color gradient transitioning from a yellow/orange hue in the core to a slightly bluer shade in the outer regions, suggesting recent, albeit minimal, star formation is occurring. The overall symmetrical and homogenous structure indicates the system is relatively undisturbed, without prominent tidal features or significant asymmetries. It possesses an estimated mass typical of large galaxies. The relatively low rate of star formation suggests that the galaxy is a relatively quiescent system.
