The galaxy appears to be a relatively smooth, elliptical galaxy. The central bulge is prominent and appears uniformly bright, indicative of a high concentration of older stars. There is a slight elongation along one axis, suggesting it may be classified as an E3-E5 on the Hubble scale. The overall color is yellowish, suggesting a population of older stars with a low rate of ongoing star formation. There is a very subtle indication of a disk. No distinct dust lanes or spiral arm structures are visible. Overall, the galaxy exhibits a well-defined and undisturbed morphology. There may be faint signs of disturbances due to a minor merger, but the galaxy is primarily undisturbed.
