The galaxy presents as a centrally concentrated, relatively smooth elliptical system. Its overall morphology is quite regular, exhibiting a high degree of circular symmetry. There is no visible evidence of spiral arm structures or a prominent disk. The light distribution suggests a centrally dominant bulge, with a smooth decrease in intensity from the core outwards. The core exhibits a bright, condensed nucleus, with a hint of blue shifting to red in the outer layers. The color gradient and smooth morphology indicates that the galaxy is most likely at a moderate redshift. The galaxy may be undergoing some star formation, though at a low rate, based on the colors. There appear to be no signs of tidal disturbances or ongoing mergers.
