The galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology. The prominent dust lane bisects the galaxy, obscuring the central bulge and imparting a distinct color gradient across the disk. The light distribution suggests an exponential profile. The overall shape is elongated, with axial ratio indicating a significant degree of flattening. One companion galaxy, possibly undergoing interaction or tidal disturbance, is apparent in the vicinity. Traces of faint, diffuse light are observed extending from the main galactic body, suggesting a possible tidal feature or stellar halo.
