The galaxy exhibits a morphology consistent with a spiral galaxy, though it is tilted nearly edge-on relative to our line of sight. The disk appears prominent. The central bulge is not dominant and may be small relative to the overall disk size. Two spiral arms are clearly discernible, appearing loosely wound. There is evidence of ongoing star formation indicated by the blue hues along the spiral arms. No signs of a strong bar structure are observed within the central region. The galaxy does not appear to be undergoing a major merger, though some minor disturbances within the disk cannot be ruled out. The overall shape is not completely smooth, but rather exhibits features associated with spiral arm structure.
