The galaxy presents as a centrally concentrated, elliptical-like structure. Its overall color profile is a blend of light yellows and whites, suggesting an older stellar population. The outer regions exhibit a faint, diffuse halo. There is no apparent spiral arm structure or significant dust lane features visible in this image. The galaxy's smooth morphology indicates it is likely in a relatively undisturbed state, with no major ongoing merger events strongly suggested. There may be a slight inclination relative to our line of sight.
