The galaxy appears to be a spiral, viewed at a fairly high inclination. There is a prominent bulge that transitions smoothly to the disc. There is likely some dust, perhaps a weak bar and hints of flocculent spiral arms. The disk is composed of a field of both young blue stars and older red stars. There is some indication of recent star formation, but perhaps a relatively low rate. The galaxy does not appear to be undergoing any major merging events, though minor interactions or disturbances cannot be ruled out. The bulge appears to be composed of older stars. The morphology seems to be somewhere between a elliptical and spiral, but leans heavily towards spiral.
