The galaxy presents as a relatively smooth, elongated structure. It exhibits a dominant central bulge region, characterized by a yellowish-white hue, suggesting an older stellar population. Proceeding outward from the bulge along the major axis, a disk-like component is visible, albeit with a shallow viewing angle. The disk shows evidence of some blue color, suggesting the presence of younger, hotter stars, and ongoing star formation.

The overall shape of the galaxy is strongly cigar-shaped, lacking a well-defined spiral structure within the observed color bands. There are no significant signs of major mergers or tidal disturbances. The morphology suggests a relatively undisturbed system, with potentially low-level star formation activity concentrated within the disk.
