The galaxy presents as a fairly compact and luminous structure. It appears largely smooth and elliptical in shape, with a high degree of roundness. There appears to be little in the way of defined spiral arms or a prominent disk structure. Faint tidal tails and minor disturbances seem to be present, suggesting a past or ongoing interaction with another galaxy. A potential merger with a smaller object may be occurring, given the disturbed structure and lack of clarity in the outer regions. The galaxy’s core presents as bright and concentrated, while color gradients suggest variations in stellar populations.
