The galaxy presents a largely smooth morphology with a hint of disk-like structure. The overall shape is generally round, with slight deviations from perfect circularity. There is no strong indication of significant ongoing merging activity, although minor disturbances cannot be ruled out. The galaxy has a prominent central bulge that is slightly elongated, with a color profile indicating older stellar populations. The disk component is subtle, showing less intense light output compared to the bulge, and no spiral arm features are readily visible. The color suggests a population of evolved stars, indicating a low rate of current star formation.
