The galaxy presents as a relatively face-on spiral, though the inclination obscures some of the finer details. There is evidence of well-defined spiral arm structure extending from a central bulge. The arms appear somewhat flocculent and show signs of ongoing star formation. A subtle bar feature seems to be present in the central region. The bulge component appears relatively small compared to the overall disk size, and the galaxy may be undergoing some minor merger activity. The stellar population in the disk component appears generally younger and bluer.
