The galaxy appears to be a spiral galaxy exhibiting a prominent disk structure. Two spiral arms are visible, one more tightly wound, and another appearing more diffuse and patchy. The arms show hints of active star formation regions, exhibiting a bluer hue compared to the rest of the disk. The galaxy possesses a notable bulge, which is medium in size and has a strong concentration of light, suggesting an older stellar population. There may be a slight indication of a bar-like feature, however it cannot be classified as a strong bar. The galaxy shows a sign of a minor disturbance or possible tidal interaction with another object, but could also just be an irregular morphological feature within one of the spiral arms.
