The galaxy appears as an elongated, spindle-shaped object. It exhibits a smooth, diffuse morphology with a concentrated central bulge that fades into a less-defined outer region. The color gradient suggests a higher concentration of older stellar populations in the core, shifting toward bluer hues in the less dense regions, indicative of younger star formation. There is no clear evidence of spiral arm structure or significant dust lanes. The overall appearance suggests a disk galaxy viewed at a high inclination, nearly edge-on. Minor irregularities in the light distribution hint at potential past interactions. 
