The galaxy displays a distinct spiral structure, with two prominent spiral arms emanating from a central region. These arms appear relatively tightly wound around the center. The overall appearance suggests a relatively large bulge, which is neither dominant nor non-existent. The bulge appears moderate in size. The presence of significant disturbances is evident. The galaxy appears to be undergoing some form of interaction, suggesting a possible minor disturbance or even a merger event. There does not appear to be a strong bar structure present.
