The galaxy presents as a relatively smooth and rounded object, with a centrally concentrated light profile. The core exhibits a bright, compact region which gradually diffuses outwards. There is little evidence of spiral arm structure or significant dust lanes. The object is approximately 3 kiloparsecs in radius. The color is primarily a pale blue, with some green, suggesting a mix of stellar populations with some ongoing, but low, star formation. There are no signs of major mergers or significant tidal disturbances.
