The galaxy presents as a spiral type with visible spiral arm structure. The arms appear to be loosely wound. There is some evidence of a bar structure, although it is not pronounced. The central bulge is not particularly dominant, appearing to be more of a moderate size, however this assessment is limited by image quality. Star formation seems to be occurring within the spiral arms, indicated by the bluer color, while the more central regions appear yellower in comparison. There is an apparent distortion in the overall morphology, which could suggest a recent or ongoing interaction or merger with another galaxy. Some areas show signs of significant disturbance.
