The galaxy presents as a relatively smooth, centralized object. Its shape is largely elliptical, with a high degree of roundness. There is a noticeable color gradient, transitioning from a brighter, yellowish-white core to a bluer outer region. There is no obvious presence of defined spiral arms or a distinct disk structure. Based on the lack of significant visual distortions and the high smoothness fraction, the galaxy is likely not undergoing a major merger event, though there may be some minor disturbances.
