The galaxy presents as a generally smooth, elliptical morphology with a highly concentrated central bulge exhibiting a bright, yellowish-white core. Moving outward from the center, the galaxy's luminosity gradually decreases, transitioning to a less intensely colored halo. The outer regions of the halo appear somewhat elongated, displaying a subtle but noticeable asymmetry in the overall shape. There is no clear evidence of spiral arm structures or prominent dust lanes. The galaxy appears relatively undisturbed, lacking any obvious signs of recent major merger activity, although subtle disturbances may be present. Overall, the galaxy exhibits characteristics consistent with a relatively massive, evolved system with a minimal rate of current star formation.
