The galaxy appears as a yellowish, elliptical structure. There is a bright, concentrated central bulge, which gradually diffuses outwards. The overall form is smooth, with minimal indication of spiral arms or significant dust lanes. The shape deviates from a perfect circle, showing a slight elongation that suggests a prolate spheroid shape. There may be minor signs of disturbance, though the primary structure seems relatively undisturbed. The color profile implies a predominantly older stellar population with little active star formation within the central region. The outer regions demonstrate a slight blue tint, suggesting some recent star forming regions on the outer rim.
