The galaxy presents as a relatively smooth, disk-shaped structure with an elongated morphology. The central region exhibits a concentration of light, appearing yellowish-orange, possibly indicating an older stellar population. Surrounding this core is a greenish hue, suggesting the presence of ongoing star formation. The overall structure shows minimal signs of major disturbances, like galactic mergers, but might have some minor disturbances. It is difficult to resolve any distinct spiral arm structures with the available resolution. The shape appears more cigar-like, tending away from perfectly circular.
