The galaxy presents as an elongated, disk-like structure. Its color gradient suggests an older stellar population, with a yellowish central bulge and a more diffuse, indistinct disk. The apparent lack of spiral arms or prominent dust lanes indicates a relatively smooth morphology. The galaxy appears to be edge-on or nearly edge-on, based on its highly flattened shape. There is no clear indication of any ongoing major merger activity or significant tidal disturbance in this image. Overall, it appears to be a well-defined, relatively evolved galaxy with moderate star formation.
