The galaxy appears as a relatively smooth, elliptical-like structure with a moderately elongated shape. It exhibits a central concentration of light, with a gradual decrease in luminosity towards its outer regions. While there's no clear evidence of spiral arms or a prominent disk, a subtle color variation is observed, possibly indicating differing stellar populations within the galaxy. The overall color appears to be in the redder part of the spectrum, which might suggest an older stellar population or a considerable amount of dust obscuring bluer, younger stars. There are hints of minor disturbances, though no major interactions or mergers are evident, suggesting it is a relaxed galaxy without any currently ongoing mergers.
