The galaxy presents a generally smooth morphology. Its shape is largely spheroidal, appearing highly rounded. There is little evidence of a disk or spiral arms. No major distortions or signs of ongoing merger activity are apparent. The galaxy is characterized by a central concentration of light. Color gradients suggest a change in stellar populations between the central regions and the outer parts of the galaxy. The central region emits stronger in the G and R bands, but the overall color is more prominent in the Z band, indicating a population of evolved stars and potentially some dust extinction. The galaxy appears to be relatively quiescent in terms of star formation activity. 
