The galaxy presents as an elliptical or lenticular type, exhibiting a predominantly smooth and featureless morphology. Its shape is generally in between round and elongated, not particularly cigar-shaped. The central region appears brighter and more concentrated, suggesting a significant stellar population or possible active galactic nucleus. Faint blue tinges are detectable near the edge of the galaxy, hinting at some ongoing, yet low level star formation. There is no indication of a major merger, but some minor disturbances appear present. The overall structure suggests an evolved system with a considerable mass.
