The galaxy exhibits an elliptical morphology with a high degree of smoothness, suggestive of an early-type galaxy. The central region displays a bright, concentrated core, indicating a significant stellar density. Moving outward from the core, the luminosity gradually decreases. The isophotes appear to be generally elliptical, although there is a subtle deviation from perfect ellipticity.

A faint blueish and greenish color gradient extends from the central region towards the outer edges of the galaxy. There is no sign of prominent spiral arms or a distinct disk structure. Subtle asymmetries or minor disturbances may be present, but are not immediately obvious. The galaxy does not appear to be undergoing a major merger or significant interaction with another galaxy based on its global morphology. 
