The galaxy presents as an elongated, spindle-shaped structure. Its light profile appears relatively smooth, with a subtle color gradient observed along its major axis. The core region displays a slightly more concentrated yellowish hue, transitioning gradually towards fainter, bluer tones at the outer edges. This color variation potentially indicates differing stellar populations and age gradients within the galaxy.

The apparent lack of distinct spiral arm structures and the overall smoothness suggest this galaxy may be an elliptical or lenticular type, viewed edge-on. The absence of obvious dust lanes further supports this morphological classification. It also appears to be a relatively isolated galaxy. 
