The galaxy presents as a highly elongated, likely disk-shaped structure seen at a steep inclination. It exhibits a smooth, diffuse appearance, lacking readily discernible spiral arms or a prominent central bulge. The light distribution transitions gradually from the core outwards, with a lack of distinct features. Color gradients are subtle, with a faint bluer hue towards one edge and a redder hue towards the center. This could indicate a variation in stellar populations, dust content or star formation activity. The overall morphology is consistent with a late-type spiral galaxy or possibly a lenticular galaxy with a flattened profile. There is no obvious indication of major mergers or significant tidal disturbances in this image.
