The galaxy displays a pronounced disk structure. Evident spiral arms are observed, exhibiting a tightly wound morphology. A substantial bulge component is present, though it appears to be moderate in size compared to the disk. There is visual evidence of a merging event. The system shows a primary galaxy, which appears relatively undisturbed, gravitationally interacting with a smaller companion galaxy which is significantly more distorted. There is also evidence of a tidal bridge linking the two galaxies. Dust lanes may be present within the spiral arms, though the image resolution limits definitive confirmation. The galaxy exhibits a yellowish hue, suggesting an older stellar population, especially prominent in the central bulge.
