The galaxy presents a predominantly smooth, elliptical morphology. Its core exhibits a concentrated, bright, yellowish hue, suggesting an older stellar population dominating the central region. The outer regions appear less luminous, displaying a slight bluish tint indicating the presence of some younger, bluer stars or active star formation in the galactic disk. Although generally smooth, there is subtle evidence of a flattened disk-like structure or faint spiral arms. There is no clear indication of a major ongoing merger, though minor disturbances or tidal features cannot be ruled out. Overall, the galaxy appears relatively undisturbed and evolved.
