The galaxy presents as a slightly elongated, disk-like structure. Its morphology appears relatively smooth, lacking prominent spiral arms or distinct features. The central region exhibits a brighter, concentrated luminosity suggesting the presence of a galactic bulge. A subtle color gradient is noticeable, with the central bulge showing a more yellow-orange hue, potentially indicating an older stellar population, while the outer regions display a slightly bluer tinge, suggesting more recent star formation. The overall shape is moderately elliptical, exhibiting a degree of flattening. There is no immediately obvious evidence of a major ongoing merger, although some minor disturbances or interactions cannot be entirely ruled out based on this single image.
