The galaxy appears to be a spiral galaxy with a prominent disk. Spiral arms are visible, although somewhat tightly wound, with a moderate amount of branching. The central bulge is relatively small, presenting a smooth, yellow-orange hue indicating an older stellar population. The spiral arms exhibit a bluer coloration, suggestive of ongoing star formation. The overall structure indicates some asymmetry, possibly due to minor gravitational interactions or internal dynamics. There is no clear evidence of a strong bar feature. The galaxy does not appear to be undergoing a major merger, though there may be evidence of minor disturbances in the morphology of the spiral arms.
