The galaxy presents a disk-like morphology with discernible spiral arm structure. The spiral arms are well-defined, tracing a clear pattern as they extend from a central bulge region. The winding of the spiral arms appears to be of medium tightness. The bulge exhibits a moderate size relative to the overall disk, and shows a clear bar structure. The overall color of the galaxy appears to be bluish, suggesting the presence of ongoing star formation. However, the low signal to noise ratio from the image makes it difficult to discern more features. There's no clear evidence of major merging activity or significant tidal disturbances, although minor disturbances cannot be ruled out due to the image resolution.
