The object presents as an elliptical galaxy, exhibiting a generally smooth morphology with no immediately obvious spiral arms or a distinct disk structure. Its overall shape is quite round, appearing almost spherical in projection, with only slight deviations toward an elongated form. The galaxy's light distribution appears relatively even throughout its body, though there seems to be a concentration of light near its center, indicative of a possible galactic nucleus. There may be some minor disturbances in the galaxy, possibly due to a small disturbance from a minor merger, though it mostly does not look like it has been through any major interactions. There are some visible color gradients within the galaxy. The central region appears more concentrated in bluer wavelengths, while the outer regions become more red, suggesting older stellar populations. The overall brightness and size of the galaxy indicate it is a fairly massive object, showing star formation may be occurring at a fairly low rate.
