The galaxy presents an elongated, edge-on disk morphology. A central bulge is apparent, exhibiting a smooth texture and a color gradient that shifts toward redder wavelengths in comparison to the rest of the disk. This suggests an older stellar population within the bulge. The disk itself shows a relatively smooth, even distribution of light, with a noticeable color gradient from bluer at the edge to redder towards the center. A relatively small amount of star formation may be occurring. There is no evidence of strong spiral arm structure. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or interactions.
