The galaxy presents as a somewhat elliptical, relatively smooth structure. The central region exhibits a concentration of light, appearing more yellow in color, which may indicate an older stellar population or significant dust obscuration. Moving outward from the core, the color transitions to a bluer hue, potentially indicative of younger stars in the galactic disk. There are no clear spiral arm structures visible, though faint, subtle asymmetries suggest the presence of some internal features or minor disturbances. Overall, the galaxy appears to be a relatively undisturbed system.
