The galaxy presents as a disk galaxy, viewed almost perfectly edge-on. There is evidence of a central bulge component, appearing somewhat elongated and with a smooth profile. The disk is relatively thin and shows only subtle colour variations, indicating a moderate amount of ongoing star formation across the plane of the disk. The bulge exhibits a yellowish hue, potentially indicative of an older stellar population. There is no obvious presence of strong dust lanes or significant distortions in the disk, suggesting a relatively undisturbed morphology. The galaxy does not appear to be currently undergoing a major merging event, although the minor asymmetry cannot rule out a past merger event.
