The galaxy presents as an elliptical morphology, exhibiting a generally smooth and featureless appearance. It appears well-rounded, deviating minimally from a circular shape. The color profile is dominated by redder hues, concentrating toward the center and gradually fading outward. The overall light distribution suggests a centrally concentrated stellar population. There is no evident sign of strong spiral arm structures, prominent dust lanes, or active galactic nucleus activity. The galaxy does not display major distortions suggestive of a recent or ongoing merger, but there is subtle evidence of some minor asymmetry. The galaxy appears to be a relatively quiescent system with little ongoing star formation.
