The galaxy presents as a well-defined, elongated structure with a distinct central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Extending outwards from the bulge, fainter, bluer regions are visible. The morphology appears largely smooth, with minimal evidence of strong spiral arms or significant disturbances. There is a hint of a disk-like structure oriented along the major axis of the galaxy. The overall shape is somewhat cigar-shaped, with the light appearing concentrated in the center.
