The galaxy presents as a slightly elongated, elliptical form. Its central region exhibits a higher surface brightness, appearing relatively smooth with a distinct reddish hue. The outer regions display a decrease in surface brightness and a slightly bluer tint, possibly indicating the presence of younger stellar populations. There are no immediately obvious spiral arm structures or prominent dust lanes visible. The overall morphology suggests an evolved system, potentially an elliptical galaxy, or a late-stage spiral transitioning to a lenticular type. There is no evidence of recent major mergers or significant tidal disturbances. The galaxy appears fairly isolated.
