The galaxy presents as an elongated, disk-like structure, oriented nearly edge-on relative to our line of sight. The central region exhibits a yellowish-orange hue, suggesting an older stellar population and possibly a significant bulge. This contrasts with the fainter, bluish-white light emanating from the outer regions of the disk.

Dust lanes appear to traverse the disk, especially near the central region. These dust lanes contribute to the patchy and somewhat irregular appearance of the galaxy. The overall morphology suggests a spiral galaxy, although the edge-on orientation obscures any clear spiral arm structure. There is no evidence of tidal tails or other major disturbances. The galaxy appears relatively isolated, with no obvious companion galaxies or signs of recent merger activity.
