The galaxy presents as an elongated, edge-on spiral, or possibly lenticular, system. A central bulge is visible, exhibiting a smoother texture and a slightly brighter concentration of light compared to the surrounding disk. The disk itself is thin and elongated, with some suggestion of dust lanes, though the resolution is insufficient for clear delineation. The light emitted from the disk appears bluer in hue, possibly indicative of ongoing, but not extremely high, star formation activity. There is no significant evidence of tidal tails, strong gravitational lensing, or major merger activity in this image. The morphology suggests a relatively undisturbed disk galaxy observed edge-on.
