The galaxy presents a relatively smooth, elliptical morphology, with a distinct central bulge that appears brighter and more concentrated than the outer regions. The color gradient suggests an older stellar population, with the central bulge exhibiting a yellowish-orange hue, possibly indicating a higher abundance of evolved stars. There is a faint, diffuse halo surrounding the main body of the galaxy, which gradually fades into the background. The overall structure appears undisturbed, showing no obvious signs of major mergers or tidal interactions. There are hints of faint, disk-like features with some mild disturbances.
