The galaxy presents a generally smooth and rounded morphology, exhibiting a structure that appears largely undisturbed. The light distribution suggests a centrally concentrated spheroid, potentially indicative of an elliptical galaxy or a lenticular galaxy viewed face-on. There is a subtle color gradient with a slightly yellower core. This might indicate an older stellar population concentrated towards the center, with a reduced rate of star formation. No distinct spiral arms or bar structures are discernible.
