The galaxy presents as a spiral galaxy with a notable disk structure. While not viewed edge-on, the disk is significantly inclined. Spiral arms are present, though not sharply defined. The central bulge appears relatively small, with no bar clearly visible in the image. The spiral arms are moderately wound. There is no obvious evidence of a major merger, though some minor asymmetry might suggest possible interaction or internal disturbance. Overall, the galaxy appears to be undergoing active star formation, which may be driving the observed spiral structure.
