The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a generally round morphology. It presents a concentrated central bulge that appears to be uniformly colored. There is a hint of a disk-like structure, although its features are subtle. The overall color is consistent with an older stellar population, and the galaxy is likely to have a substantial mass. There is no evidence of any major ongoing merger events, but some minor distortions and a small fraction of merging cannot be ruled out. Star formation activity appears to be very low.
