The galaxy presents as a somewhat diffuse and elliptical structure. It appears to be relatively smooth, with a brighter, concentrated central region. The outer regions exhibit a more dispersed profile. Subtle hints of a disk-like structure are suggested by the slightly flattened shape. There may be some minor disturbances or interactions occuring. No strong evidence of spiral arms is visible; the color suggests ongoing star formation, particularly in the central region. The overall morphology suggests a galaxy somewhere on the elliptical-to-spiral transition.
