The galaxy presents as a spiral type, observed at a steep inclination, nearing edge-on. A prominent central bulge dominates the structure, exhibiting a concentrated luminosity. The disk is readily apparent, extending laterally from the bulge. There are some dusty regions throughout the disk, but they do not appear to be very clumpy and star formation seems to be mostly homogeneous.

In color imagery, the bulge appears yellowish-orange. The disk appears to have some blue in it, and the yellowish-orange color becomes white towards the edge of the disk. This suggests an intermediate age stellar population throughout the galaxy. There appears to be low levels of ongoing star formation in a spiral structure. 

The overall morphology is largely undisturbed, although there is a possibility of minor asymmetries indicating past interactions or internal instabilities. No major merger signatures are visible.
