The galaxy presents as a spiral type, with a noticeable disk structure viewed at an oblique angle. Spiral arms are visible, exhibiting a somewhat patchy and flocculent morphology. A central bulge is prominent, displaying a moderate size relative to the disk. There is evidence of a possible bar feature traversing the central region. The galaxy's color suggests ongoing star formation, particularly in the spiral arms, evidenced by their bluer hues. The overall structure appears relatively undisturbed, without strong signs of a recent major merger, although a minor interaction cannot be ruled out due to some apparent asymmetry in the disk.
