The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are well-defined and appear loosely wound, with a dominant two-arm structure. There is evidence of a bar-like feature spanning the central region of the galaxy. A moderate bulge is observed, though it appears smaller compared to the overall size of the disk. The galaxy shows signs of tidal disturbance and/or possible interaction with another galaxy. A possible merging event may be present. There are areas of high star formation visible in the spiral arms.
