The galaxy presents as a spiral, viewed at an oblique angle, likely with a redshift of approximately 0.049. It exhibits a disk structure, and appears to be the dominant feature of the system. Spiral arms are clearly visible, showing a winding pattern that ranges from tightly wound to more open structures. The color distribution suggests ongoing star formation within the arms, evident from the bluer hues. The central bulge shows a moderate size. There appears to be a weak bar-like feature crossing the central region, but its presence is not prominent. The overall morphology suggests that the galaxy is not currently undergoing any major merger events, although minor disturbances cannot be ruled out.
