The observed galaxy presents as a flattened, elongated structure, oriented nearly edge-on relative to our line of sight. The dominant color is a yellow-orange hue, suggesting an older stellar population. There's a subtle color gradient visible, with a somewhat reddish tint concentrated toward the central region, possibly indicating the presence of dust obscuring a fraction of the starlight or regions of on-going star formation. The lack of clearly defined spiral arms or distinct features suggests that this galaxy is likely a disk galaxy, probably an actively star-forming spiral galaxy. The lack of strong irregularities in the morphology suggest no recent major merger events.
