The galaxy presents a largely smooth and elliptical morphology. Its core is intensely luminous, exhibiting a concentrated brightness profile that gradually diffuses outwards. There is a noticeable radial color gradient, transitioning from a yellowish-white core to a slightly bluer and fainter halo. The overall structure appears undisturbed, lacking any prominent tidal features or signs of ongoing major mergers. Based on the morphology, it appears to be an early-type galaxy, potentially an elliptical or lenticular. Faint hints of underlying structure might suggest the presence of a weak disk or minor features, but the dominant impression is one of smoothness and symmetry. The lack of distinct features suggests that the star formation rate is likely low.
