The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge. These arms display a loosely wound structure. A stellar bar crosses the bulge. The bulge appears moderately sized relative to the overall galactic disk. The galaxy exhibits a redder hue towards the central bulge, suggesting an older stellar population. Distortions are visible in the spiral arm structure; however, no strong signs of a major merger are observed. The disk shows evidence of ongoing star formation, indicated by the presence of bluer regions within the spiral arms.
