The galaxy presents a largely smooth morphology, with a high degree of central concentration. Its overall shape appears predominantly round. There is no obvious indication of strong spiral arm structure or a prominent disk. The light is dominated by a yellow-white hue, suggesting an older stellar population. Faint blue tinges may imply slight traces of ongoing, yet low-level, star formation within the galaxy. No signs of an ongoing major merger are evident; however, a minor interaction or disturbance cannot be entirely ruled out given the fuzzy edges.
