This galaxy appears to be a spiral galaxy, viewed at an angle close to face-on. It exhibits a central bulge, and a disk structure with spiral arms that are visible. The spiral arms are moderately wound, neither tightly coiled nor loosely extending. There is some evidence of a bar-like structure intersecting the central bulge. The bulge itself does not seem to be particularly dominant, appearing to be of moderate size compared to the disk. There is a distinct color gradient across the galaxy, with the central regions appearing more yellowish-white, transitioning to bluish hues in the outer spiral arms. This may indicate variations in stellar populations. The spiral structure is somewhat flocculent. Overall, there are some indications of minor disturbances in the galaxy's structure, but nothing to suggest this is the result of a significant ongoing merger event.
