This galaxy presents a clear edge-on disk morphology. A prominent central bulge dominates the galactic structure, exhibiting a smooth and diffuse light distribution, potentially indicative of an older stellar population. The disk component appears relatively thin and elongated, with the primary axis spanning approximately 4.3 arcseconds.  Subtle color gradients suggest potential differences in stellar populations between the bulge and the disk, with the bulge appearing slightly more yellow, and the disk a bit bluer. Evidence of recent major merging events is absent.
