The galaxy presents as an elongated, disk-like structure viewed at a significant angle, appearing nearly edge-on. The central region exhibits a concentration of light with a reddish-orange hue, potentially indicating an older stellar population. The outer regions of the disk are bluer, which suggests the presence of younger, hotter stars and active star formation. Although primarily smooth in appearance, there might be subtle disturbances or asymmetries present, hinting at possible past interactions or internal dynamic processes. Overall, it seems to be a relatively massive galaxy with ongoing star formation.
