The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology, tending towards being in-between rounded and elongated. The light distribution suggests a dominant bulge component, with a noticeable color gradient from the center outwards. The central region exhibits a yellowish-orange hue, potentially indicating an older stellar population. The outer regions appear fainter with a slight shift towards bluer colors, possibly hinting at more recent star formation activity. There is no apparent evidence of strong spiral arm structures or significant tidal disturbances. Overall, the galaxy's appearance is consistent with that of an early-type spiral or lenticular galaxy seen at a considerable distance.
