The galaxy appears to be a spiral galaxy, though the spiral arms are not highly defined. There is evidence of a disk structure, but it is not perfectly edge-on or face-on. The central bulge is prominent and exhibits a yellow-orange hue, suggesting an older stellar population. There is a blue-white section toward the upper end of the disk, indicating a small area of current or recent star formation. The lower area of the disk also has a hint of yellow, suggesting a mix of stellar populations. There may be some minor disturbances visible in the galaxy's morphology, though the structure remains broadly intact, which is consistent with a potential ongoing minor interaction with another galaxy.
