The galaxy presents as a diffuse elliptical, with a high degree of central concentration indicated by the bright yellowish core. The outer regions exhibit a more irregular morphology with hints of spiral arm structures. There are noticeable blue tinges, particularly in the outer regions, suggesting ongoing star formation. Overall, the galaxy appears to be relatively smooth, with no obvious signs of a major merger, but there is some indication of a possible minor disturbance in its morphology. The galaxy is slightly more extended along one axis, indicating a mild ellipticity.
