The galaxy presents a somewhat elliptical morphology. It exhibits a central bulge region that appears relatively smooth, with a moderate concentration of light. The disk component shows a discernible spiral structure, although it appears somewhat flocculent and not tightly wound. There is evidence of ongoing star formation within the spiral arms, as indicated by the presence of blue-ish hues. The galaxy does not seem to be strongly barred, but there is some degree of asymmetry or distortion present, suggesting possible minor interactions or disturbances.
