The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge, which appears nearly spherical, dominates the galaxy's core, exhibiting a yellowish-white hue, suggesting an older stellar population. Dust lanes are faintly visible within the disk, obscuring some of the starlight. The disk itself appears relatively smooth, with a distinct but subtle color gradient shifting towards bluer tones further from the central bulge, potentially indicative of ongoing star formation in the outer regions. There are minimal signs of any significant mergers or tidal disturbances. The galaxy appears relatively isolated, with a well-defined shape and structure.
