The galaxy presents as a late-type spiral galaxy, viewed almost perfectly edge-on. A central bulge is visible, with a rounded morphology and a distinct color gradient that is more yellow than the outer disk. This bulge indicates an older stellar population. A flattened disk extends outward from the bulge. The disk appears relatively smooth and uniform in color, with some faint hints of structural features along the disk, which could indicate spiral arms. The disk’s color is more blue/green than the bulge, suggesting the presence of younger stars. Overall, the galaxy appears undisturbed, with no obvious signs of a major merger or tidal interactions, though there may be a slight asymmetry in the disk suggesting a minor gravitational interaction. The galaxy appears to be actively forming stars, based on the color, but at a low rate. The physical size of the galaxy is moderate.
