The galaxy presents as a lenticular or possibly an early-type spiral with a relatively smooth, centralized bulge. The disk component is faint but discernable. The galaxy has an elongated shape, it is likely that it is observed at a high inclination angle. There's a hint of non-uniformity, possibly indicating minor disturbances or asymmetries in its structure. There are areas with faint hints of blue, possibly due to the presence of some younger stellar populations or low levels of ongoing star formation. The overall color suggests a relatively evolved stellar population.
