The galaxy presents as a centrally concentrated, largely smooth object. It exhibits a radial gradient in brightness, with a bright, well-defined core that gradually fades into a more diffuse halo. The overall shape is generally round. There is a slight hint of asymmetry in the outer regions of the halo, but no clear evidence of strong spiral arm structures or other prominent features. Color gradients are subtle, but a slight bluer hue seems present in the outer regions. No signs of major mergers or significant tidal disturbances are immediately apparent, though there may be some minor disturbances. The galaxy appears to be a relatively undisturbed system.
