The galaxy presents as a relatively compact object with a disk-like morphology, viewed nearly edge-on from our perspective. A bright central bulge is apparent, showing a high degree of concentration. Surrounding this bulge is a disk component that appears relatively thin and elongated. The disk displays some structure, hinting at the presence of spiral arms, although these are not well-defined. There is evidence of a faint, diffuse halo surrounding the main body of the galaxy. The color gradient suggests active star formation regions. Overall, the galaxy appears to be a spiral galaxy exhibiting signs of interaction or disturbance. 
