The galaxy presents as a lenticular or early-type spiral galaxy. It appears relatively smooth in texture and shows a subtle disk-like structure. The major axis is moderately elongated, transitioning between a circular and cigar-like shape. There is no strong evidence of significant ongoing merger activity or major tidal disturbances. There may be minor disturbances or interactions, but the main body appears mostly relaxed and undisturbed. The color suggests the presence of an older stellar population with minimal ongoing star formation.
