The object appears to be a spiral galaxy, viewed at an oblique angle, nearly edge-on. A central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. Faint and diffuse spiral arms extend outward from the bulge, displaying a bluer color, possibly indicating regions of recent star formation. The spiral arms seem loosely wound. A bar structure seems to be faintly present. The galaxy shows no major signs of ongoing merger activity, but minor disturbances cannot be ruled out based on the image. The disk component of the galaxy appears to be dominant over the bulge.
