The galaxy presents a largely smooth morphology, with minimal apparent substructure. Its overall form appears to be elliptical or lenticular. There is a radial brightness gradient increasing towards the center of the galaxy, with the galactic nucleus unresolved and appearing as a bright, concentrated point. The light distribution suggests a high degree of rotational symmetry, with no obvious signs of tidal distortions or ongoing mergers. The galaxy exhibits a noticeable red-shift, indicating a substantial distance. Color gradients are present, with the central region appearing slightly yellower compared to the outer regions, suggesting an older stellar population in the core. Overall, the galaxy appears to be a relatively evolved and quiescent system.
