The galaxy presents as a moderately inclined spiral. It exhibits a central bulge that appears relatively smooth and concentrated. The disk component is visible, but it lacks clearly defined spiral arms. There is evidence of some disk structure, possibly faint or tightly wound spiral arms, though these are not sharply resolved. The overall color is intermediate, suggesting the presence of both older stellar populations and some ongoing star formation. The galaxy appears somewhat disturbed and has a clumpy morphology.
