The galaxy presents as a disk galaxy, observed nearly edge-on from our line of sight. There is a central bulge that appears bright and concentrated, suggesting a relatively high stellar density in this region. Dust lanes are likely present within the disk, contributing to the galaxy's redder hue. The disk appears relatively smooth, lacking prominent spiral arm structures; however, it is difficult to assess its precise morphological classification due to the edge-on orientation. No major disturbances are seen, so it seems it is relatively undisturbed.