The galaxy presents as an elongated, disk-shaped structure viewed edge-on. The central region exhibits a concentrated, bright glow, suggesting a high density of stars. Fainter material extends outwards from this core, forming a flattened disk. The dust lane bisecting the disk is quite dark and wide. The disk's extremities appear fuzzy and indistinct, with a general lack of defined spiral arm structures visible at this resolution, although some subtle irregularities might be present. There is no evidence of a recent major merger.
