The galaxy presents as a somewhat smooth, disk-like structure, though the image resolution makes finer details difficult to discern. It exhibits a central bulge that appears significantly brighter and more concentrated than the outer regions. The bulge displays a yellowish-orange hue, suggestive of an older stellar population dominating this region. The disk shows a more diffuse structure, with a subtle color gradient moving outwards from the bulge. The outer disk appears to be bluer than the bulge, potentially indicating younger, hotter stars. There is a slight distortion, or minor disturbance, apparent in the morphology of the disk.
