The galaxy presents as a somewhat elongated, diffuse object with a brighter central region. Its color is predominantly bluish, suggesting the presence of a relatively young stellar population and ongoing star formation. A subtle disk-like structure may be present, although the galaxy does not exhibit well-defined spiral arms or a prominent bulge. There is a slight asymmetry in the overall form of the galaxy, hinting at possible past interactions or minor disturbances. While the overall appearance is largely smooth, there are hints of some substructure within the brighter central region.
