The galaxy presents a disk-like morphology, viewed at an angle that is close to face-on. Two spiral arms are clearly visible, tracing a somewhat tightly wound pattern outward from the central region. The arms are not uniformly distributed; rather, the arms appear to be more prominent on one side compared to the other side. The central bulge of the galaxy appears moderate in size, not completely dominant but also not insignificant. A weak bar structure might be present across the center of the bulge, but it is not very prominent. The galaxy exhibits a clear indication of ongoing or recent interaction with another object, causing a slight disturbance in its structure. The disturbance is minor and appears to be contained on one side of the galaxy.
