The galaxy presents as a flattened, disk-shaped structure, likely an edge-on or nearly edge-on spiral galaxy. A central bulge is discernible, appearing as a concentrated region of light. The bulge exhibits a yellow-white hue, potentially indicating an older stellar population. Extending outwards from the bulge is a fainter, bluer disk. The blue color suggests regions of active star formation. Patches and irregularities are visible in the disk, perhaps indicative of spiral arm structure or dust lanes. There are some indications of possible minor tidal disturbances present. Overall, it appears to be a galaxy with ongoing, albeit perhaps not exceptionally high, levels of star formation.
