The galaxy presents as a lenticular or possibly an elliptical system, with a smooth, diffuse light distribution indicative of an older stellar population. The central bulge region exhibits a yellowish-orange hue, suggesting a concentration of evolved stars. The overall shape is elongated, with a high probability of being observed from a significantly angled or edge-on perspective. There is no clear evidence of spiral arm structure or significant dust lanes visible in this imaging. Subtle color gradients are present, indicating possible variations in stellar populations or metallicity across the galaxy. There appears to be no evidence of any recent major merging events, with the object being relatively undisturbed. The morphology is broadly consistent with a passively evolving system, with low levels of on-going star formation activity. 
