The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge. The spiral arms appear loosely wound, with some patchiness, suggesting areas of active star formation. The bulge exhibits a moderate size relative to the overall galactic disk, with a smooth texture, indicating an older stellar population. There is no clear indication of a strong bar structure within the galaxy, although a faint, elongated feature may be present. The overall appearance is relatively undisturbed, with no obvious signs of a major merger event, though some minor disturbance may be present. The galaxy is observed at a redshift of approximately 0.27, placing it at a considerable distance.
