The galaxy presents as a relatively small, elongated structure. Its morphology suggests a disk galaxy viewed nearly edge-on. The central bulge exhibits a brighter, more concentrated luminosity, indicating a higher stellar density. The disk appears to be composed of older stellar populations due to its yellow-orange color and lack of distinct spiral arm structure. This, in turn, implies a low rate of active star formation across the galaxy. There is some asymmetry in the disk's shape, and the dust lane that is usually observed when viewing an edge-on galaxy is either not present, or not able to be seen at this resolution.
