The galaxy presents a largely smooth and elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The central region exhibits a high surface brightness, indicating a concentrated stellar population and possibly an active galactic nucleus. The color profile is consistent with an older stellar population, dominated by redder wavelengths, with a hint of green. The overall shape is roughly rounded, though not perfectly circular, and appears undisturbed, without major signs of ongoing merger activity. There is evidence of minor asymmetry or a slight disturbance.
