The galaxy presents a distinct spiral morphology. Spiral arms are visible. The winding of the spiral arms appears to be of moderate tightness, with a hint of a two-arm structure. A central bulge is observed; it appears to be of moderate size, with a yellowish color suggesting an older stellar population. A bar structure may be present, but it's not distinctly strong. There's no clear evidence of major mergers or significant tidal disturbances.
