The galaxy presents as an elliptical type with a generally smooth morphology. Its shape is closer to being in-between round and cigar shaped, appearing moderately flattened. There is a bright central bulge that dominates the galaxy's luminosity. Fainter regions extend outwards from this central region. There is no evidence of strong spiral arm structures or a prominent disk. No significant tidal disturbances or merging features are obviously visible, though minor disturbances cannot be ruled out. The galaxy appears to be composed of primarily older stellar populations which are concentrated in the bulge.
