The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology with a subtly elongated shape. A central bulge region shows a yellowish color, possibly indicative of an older stellar population or dust obscuration. The outer regions display a more bluish-green hue, suggesting the presence of younger, hotter stars. There is little discernible structure such as spiral arms or a prominent disk. The galaxy does not appear to be significantly disturbed or undergoing a major merging event.
