The galaxy exhibits a disk-like morphology and appears to be oriented close to edge-on. The disk displays a noticeable bulge, though it is difficult to discern the bulge's detailed structure at this resolution. There is evidence of internal structure within the disk, as seen by the uneven light distribution. There also appears to be minor irregularities within the disk, though no prominent or major disturbance seems to be occurring. The color suggests ongoing star formation activity.
