The galaxy presents as a slightly inclined, elongated structure. The central region exhibits a higher surface brightness and a yellowish hue, suggesting a concentration of older stellar populations. The outer regions appear more diffuse and bluer in color, which could indicate the presence of younger, hotter stars and ongoing star formation. There's a subtle hint of a possible spiral arm structure on one side, though it is not clearly defined. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event. It is possibly a spiral galaxy that is being observed edge on.
