The galaxy presents an elliptical morphology, appearing largely smooth in structure with a concentrated, bright central region. A slight elongation is observed, indicating a potential departure from perfect circularity. The light distribution suggests a gradual decrease in intensity from the core outwards. Colors appear mixed but generally feature a dominant light-blue-green hue toward the center, transitioning to a redder tone around the periphery. There is no obvious presence of distinct spiral arms or a well-defined disk structure, supporting its classification as an elliptical or lenticular galaxy. Subtle irregularities in the outer regions suggest the possibility of minor tidal interactions or past merger events, though no strong evidence is visible in this imaging.