The galaxy exhibits a morphology indicative of a spiral structure, although the inclination obscures a full planar view. There is a distinct central bulge with a yellowish hue, suggesting an older stellar population. Broad spiral arms are present, exhibiting a medium winding. The arms appear to be populated by both younger, bluer stars and older, yellower stars. It seems like the galaxy is undergoing a minor merger. Overall, the structure seems like a spiral galaxy undergoing complex interactions, and the bar may be present.