The galaxy appears as a relatively compact, centrally concentrated object. There is a central bulge that is bright, but is not very distinct from the rest of the galaxy.  The galaxy exhibits a complex and potentially disturbed morphology.  A fainter, diffuse halo or envelope surrounds the brighter central region. The color is shifted toward the blue end of the spectrum, suggesting recent star formation. There is some faint structure or irregularities that might indicate a potential ongoing minor merger. The general shape appears elliptical, and possibly elongated, with a diameter of roughly 2 arcseconds.
