The galaxy presents a primarily smooth morphology. Its shape approximates an elliptical form, appearing largely round with only a subtle deviation toward a more elongated, cigar-like appearance. The central region exhibits a concentrated brightness, indicative of a substantial stellar population or active galactic nucleus. There is a noticeable lack of spiral arm structures or prominent dust lanes. Faint color variations are present, with a dominant yellowish-orange hue in the center, which potentially signifies an older stellar population. The outer regions appear to be subtly bluer. There is no apparent evidence of any major ongoing mergers, or significant tidal disturbances, although there may be subtle asymmetry in the light distribution. Overall, the galaxy appears to be a relatively undisturbed and potentially evolved system.
