The galaxy presents as a somewhat elliptical structure with an apparent disk, with a slight elongation. The light distribution appears relatively smooth, with a brighter, more concentrated central region that fades gradually into the outer regions of the galaxy. There is a hint of asymmetry in the outer regions, suggesting possible tidal interactions or disturbances. Color gradients are visible; the central region appears more yellow/orange, indicating an older stellar population or dust obscuration, while the outer regions show a bluer hue, possibly indicating the presence of younger, hotter stars. There is a distinct blue region to one side, this suggests the galaxy is forming new stars in that location. Overall, the galaxy appears to be relatively evolved, with ongoing but perhaps declining star formation.
