The galaxy presents as a spiral type, viewed at an angle slightly offset from face-on. Prominent spiral arms extend from a central region, showing a relatively tightly wound structure. At least three spiral arms can be identified. A hint of a bar-like structure is suggested across the central bulge, though not distinctly defined. The bulge itself appears relatively small compared to the overall disk size. 

The arms are visibly bluer in color, indicating regions of ongoing star formation. The overall morphology suggests a galaxy that is not currently undergoing a major merger, though some minor disturbances or tidal features could be present within the structure. A flocculent appearance is noted along the spiral arms with varying densities.
