The galaxy presents as a disturbed spiral morphology, characterized by a distinct, elongated shape suggestive of an ongoing or recent interaction with another galaxy. The spiral arms are loosely wound and ill-defined, showing signs of disruption and tidal forces. The overall color of the galaxy is a yellowish hue, with pockets of bluer regions interspersed throughout the spiral arms. This implies a combination of older stellar populations and areas of active star formation. There may be a presence of a bar structure, but this is difficult to observe due to the disturbance of the arms. A bulge component is visible, but not very prominent. A large portion of the light comes from the central portion of the galaxy. Evidence of an apparent tidal tail can be seen near the galaxy, further supporting the occurrence of a merger.
