The galaxy presents as a centrally concentrated, smooth object, appearing largely featureless across the observed wavelengths. The light distribution is roughly circular, exhibiting a high degree of central symmetry with a gradual falloff in intensity from the core to the outer regions. There is no apparent disk structure or spiral arm morphology. The galaxy displays a subtle color gradient, with a slightly bluer hue towards the center compared to the redder, fainter periphery. Minimal signs of recent or ongoing major mergers are present, though the slight asymmetry to the right indicates possible minor tidal disturbances or past interactions. The smooth profile and lack of discernible substructure suggest a relatively evolved system, possibly an elliptical galaxy. Overall the galaxy is compact, appearing dense and uniformly distributed.
