The galaxy presents a well-defined, though somewhat indistinct, spiral structure. Multiple spiral arms are visible, though their exact count is difficult to ascertain due to the image resolution. The arms appear to exhibit a mix of medium to tight winding, with variations in pitch angle observed across the disk.

A central bulge is present, exhibiting intermediate prominence relative to the overall disk. While not a dominant feature, it is clearly discernible. There is some evidence of a possible bar-like structure within the central region, though this feature is not strongly defined.

The galaxy shows signatures of blue color, indicative of recent star formation within the spiral arms. There is no visual evidence of any active galactic nucleus activity. The overall morphological appearance suggests a galaxy undergoing relatively normal spiral galaxy evolution. Minor disturbances are potentially present in the spiral arms and overall structure.