The galaxy presents as a somewhat elongated, disk-like structure, viewed at a moderate inclination. Its central region exhibits a noticeable concentration of luminosity, appearing smooth and featureless. The outer regions display a more diffuse and less structured distribution of light. There's a suggestion of spiral arm structure but this is difficult to confirm given the image quality. The overall color is relatively uniform, trending towards redder wavelengths. There is no apparent evidence of ongoing major mergers or strong tidal disturbances.
