The galaxy presents a complex morphological structure, appearing as a distorted disk system. A significant portion of the galaxy exhibits a relatively smooth, diffuse appearance, but with some noticeable irregularities. There is a substantial amount of blue light, indicative of active star formation. The overall shape does not conform to a classical elliptical or spiral morphology, showing signs of a possible interaction or merger.

Distinct regions within the galaxy display differing levels of intensity, suggesting variations in stellar density and/or dust obscuration. An apparent bulge is either absent or minimal. Clear evidence of a well-defined spiral arm structure is lacking, but hints of disrupted spiral arms may be present. There is evidence of a major disturbance and potential merging activity.
