The galaxy appears to be largely smooth and elliptical in shape, with a generally round morphology. There is a concentration of light towards the center, suggesting a bulge. The galaxy exhibits a color gradient, transitioning from bluer hues in the inner regions to redder tones towards the outer edges. While smooth, there appears to be some subtle disruption in the overall light distribution, hinting at possible minor interactions or internal disturbances. The general symmetry suggests it is not undergoing a major merger, however a small amount of disruption can be seen. Overall, the galaxy appears to be dominated by an older stellar population.
