The galaxy presents as a flattened disk-like structure, with a major axis significantly larger than its minor axis. It exhibits a prominent central bulge that appears smooth and concentrated. The disk component shows some evidence of spiral arm structure.

In terms of color, the central bulge appears redder than the disk. The disk shows bluer regions, particularly in the outer parts of the arms, suggestive of ongoing star formation. There is also a distinct redder, circular patch in the disk itself which may be a separate object superimposed over the galaxy.

Overall, the galaxy's light distribution is dominated by the bulge, suggesting that it is an intermediate or late-type spiral galaxy. The ellipticity of the disk is substantial, and the position angle indicates a specific orientation on the sky.
