The galaxy appears to be a spiral type, exhibiting prominent, loosely wound arms. A relatively small bulge is visible in the central region. There is evidence of ongoing interaction or a merger event, indicated by significant disturbances in the galaxy's morphology. Extended tidal tails are apparent, suggesting a strong gravitational interaction. The spiral arms show signs of active star formation, as indicated by their color. It is most likely merging with another galaxy, which can be seen on the right side.
