The galaxy presents as a lenticular or early-type spiral system, appearing largely smooth and centrally concentrated. Its morphology suggests a relatively evolved state. The color index implies a population of older stars, with a subdued rate of recent star formation. The galaxy exhibits a weak disk-like structure. It is moderately elliptical in shape, not perfectly spherical, and also not a highly elongated cigar shape. There is no evidence of significant tidal disturbances or ongoing mergers in the immediate vicinity of the galaxy.
