The galaxy presents as a relatively smooth, disk-shaped structure. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the disk transitions to a bluer color, indicating the presence of younger, hotter stars. The galaxy appears elongated, with an aspect ratio suggesting it is viewed at a significant inclination. There is no clear evidence of spiral arm structure, but a faint asymmetry in the disk's outer regions hints at potential tidal interactions or past minor mergers. No significant dust lanes are immediately apparent within the disk.
