The galaxy appears to be a spiral galaxy seen at a relatively high inclination. A central bulge is visible, exhibiting a smooth, concentrated light distribution with a yellowish hue. The spiral arms are somewhat faint and diffuse, possessing a bluer color, suggesting ongoing, though perhaps not vigorous, star formation. There are no prominent signs of a major merger, although slight irregularities in the disk may indicate minor tidal interactions or internal disturbances. Overall, the galaxy presents a moderately evolved morphology.
