The object presents as a spiral galaxy, observed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. Dust lanes are apparent, though somewhat obscured, running along the galactic plane. The disk component appears relatively smooth. Hints of bluer regions are present, indicative of potential star-forming regions within the disk. No significant signs of tidal disturbance or ongoing major mergers are readily discernible.
