The galaxy presents as a lenticular or early-type spiral, with a prominent, centrally concentrated bulge. The bulge exhibits a smooth, relatively featureless appearance, suggesting an older stellar population. Fainter, diffuse disk component surrounds the bulge, viewed edge-on. There is a hint of some spiral structure close to the midplane. The dust lane appears asymmetric. The galaxy does not appear to be undergoing any major mergers, although there may be some minor disturbances. Overall, the galaxy seems to have a relatively quiescent star formation rate. The galaxy shows a redder color profile, characteristic of a more evolved system.
