The galaxy presents as an elongated structure, indicative of a disk galaxy viewed nearly edge-on. A prominent central bulge is observed, appearing relatively bright and concentrated. The bulge exhibits a rounded morphology. The disk component shows a noticeable dust lane along the central plane, obscuring light and creating a dark band that bisects the galaxy.

The overall color appears to be reddish-yellow, suggesting a population of older stars. This coloration also hints at a relatively low star formation rate within the galaxy. A distinct tidal tail emanates from one end of the galaxy, potentially caused by a past gravitational interaction. There is no apparent spiral structure.
