The galaxy presents as an elongated, edge-on disk galaxy. A prominent central bulge dominates the galaxy's core, exhibiting a smooth, relatively uniform color gradient, suggesting an older stellar population. The galactic disk displays a bluer hue and is less distinct than the bulge; there are no visible spiral arm structures. Dust lanes may be present along the plane of the disk; they appear subtle rather than sharp or well-defined. There's no obvious sign of a major ongoing merger, although some minor disturbances cannot be ruled out given the image resolution. Overall, the galaxy appears to be relatively quiescent in terms of star formation activity, which is expected for its redder color and smooth central bulge.
