The galaxy appears to be a relatively small, disk-shaped system. It exhibits a smooth, diffuse morphology, lacking prominent spiral arms or a distinct central bulge. The galaxy's color is primarily blue, suggesting the presence of a young stellar population and ongoing star formation, albeit at a moderate rate. The disk is moderately inclined with respect to our line of sight, appearing somewhat elongated. There are no obvious signs of active galactic nuclei activity, nor indications of significant recent or ongoing merger events, although some minor disturbance cannot be ruled out. The galaxy’s overall structure appears relatively undisturbed, presenting a cohesive and settled form.
