The galaxy presents a morphology consistent with a spiral structure, though near edge-on. Spiral arms are subtly discernable, exhibiting a somewhat flocculent pattern. A central bulge is visible, appearing moderate in size relative to the overall galactic disk. No strong bar structure is immediately obvious; however, a potential weak bar may be present within the inner regions of the disk. The disk component is relatively smooth, with no major signs of ongoing mergers or significant tidal disturbances. The overall color profile suggests a population of stars with a range of ages, with a bluer tinge in the disk regions possibly indicating younger stars. The central bulge appears to be a yellowish color possibly indicating older stars or dust obscuration.
