The galaxy appears to be an elliptical galaxy or a lenticular galaxy with a smooth morphology. It exhibits a near-perfectly circular profile. There is no obvious sign of spiral arms or a disk component. The light distribution suggests a centrally concentrated bulge. Evidence suggests that there is no significant ongoing merger activity or major disturbance. The galaxy's color profile indicates a lack of current star formation, with most of the light concentrated in longer wavelengths. There is a possibility of some interaction at the edge of the galaxy.
