The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a relatively smooth and concentrated structure. The central bulge is prominent and appears yellowish in color, suggesting an older stellar population. The disk is not as well-defined, showing a flattened morphology with a blue tint. The blue color potentially indicates younger stars. The galaxy does not show any prominent spiral arm structure or significant dust lanes within this image. The light appears to be evenly distributed across the disk. The galaxy appears to be isolated and does not show any signs of merging or tidal disruption.