The galaxy presents a moderately diffuse morphology, appearing as a largely smooth object with subtle internal variations in luminosity. The overall shape is neither distinctly elliptical nor spiral, tending toward a more rounded structure. There is weak suggestion of a possible disk with some mild features that might indicate minor disturbances or internal structures. The galaxy does not show obvious signs of major merger events, though more subtle interactions cannot be excluded. It shows a noticeable difference in color between the inner and outer regions, with the core appearing somewhat bluer than the surrounding areas.
