The galaxy presents as a disk galaxy observed nearly edge-on. A central bulge is apparent, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk shows a bluer tint, especially towards the edges, hinting at the presence of younger, star-forming regions, although the image resolution limits detailed morphological characterization of these regions.

The galaxy's elongated shape indicates a relatively high inclination angle with respect to the line of sight. There might be subtle disturbances visible, but without more detail, it is not possible to confirm mergers or tidal interactions. Overall, the galaxy appears relatively smooth, with a subtle disk structure.
