The galaxy presents a flattened, disk-like morphology, suggesting it is likely a spiral or lenticular galaxy viewed at an oblique angle. The central region exhibits a strong concentration of light, indicating a prominent bulge or core. The light from the bulge appears yellow-ish to red-ish, suggesting an older stellar population. The disk shows some subtle variations in brightness but lacks distinct, well-defined spiral arm structures. This could be due to the viewing angle, intrinsic faintness of the arms, or a smoother, more flocculent spiral structure. There is little evidence of strong ongoing star formation across the galaxy. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances.
