The galaxy presents as a largely featureless, smooth elliptical, or possibly lenticular, morphology. There is a distinct concentration of light toward the galactic center, indicating a bulge component. The outer regions of the galaxy appear diffuse, fading into the background. There is a slight elongation to the galaxy's shape, suggesting a moderate ellipticity rather than a perfectly spherical form. Color gradients are subtle, with the central bulge appearing somewhat yellower compared to the outer regions, potentially indicating a difference in stellar populations. There is no evidence of spiral arms or significant dust lanes. No merging features or tidal tails are discernible, suggesting a relatively undisturbed evolutionary history.
