The galaxy presents as an elliptical form, though slightly elongated along one axis. Its light profile shows a high degree of central concentration, with brightness decreasing radially outwards from the core. The central region appears to be dominated by older stellar populations, inferred from the reddish-yellow hue. Moving outwards, the galaxy exhibits a smoother texture, with an increasingly bluer tint, possibly indicating the presence of younger stars. The morphology suggests that the galaxy is relatively undisturbed, and it does not appear to be undergoing a major merger event. There is a faint, diffuse halo of light extending beyond the main body of the galaxy. No prominent spiral arms or a clear disk structure are discernible. The galaxy seems to possess a moderately smooth structure throughout, suggesting a possible lack of significant recent star formation.
