The galaxy presents a largely smooth, elliptical morphology. The core is a bright, concentrated spheroid, indicating a high stellar density. There is a color gradient within the galaxy, with the central regions exhibiting a more yellow-orange hue, suggestive of an older stellar population. The outer regions appear slightly bluer, potentially indicating the presence of younger stars or some ongoing, albeit limited, star formation. The galaxy shows a slight flattening, with a minor elongation evident in its shape. There's a hint of possible minor disturbance or interaction based on some subtle asymmetries in the outer regions. The overall structure suggests a relatively evolved system with a dominant spheroid component.
