The galaxy presents as a spiral type, observed nearly edge-on. A prominent central bulge appears bright and somewhat yellow/white, suggesting an older stellar population. The disk is visible, though tightly wound, appearing as a thin, elongated structure extending above and below the bulge. Traces of blueish color are present, indicating some level of ongoing star formation within the disk. There is a slight warping of the disk on the right side, although it could be that this is an effect of seeing the light from a distant object, not a characteristic of the shape of the galaxy. There does not seem to be any evidence of a recent major merger event. 
