The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing somewhat rounded, with a slight deviation from perfect circularity. A hint of a minor disturbance or asymmetry is visible, potentially indicating an ongoing or past interaction, or perhaps some internal process. The primary color is whitish-yellow, but it also exhibits a subtle color gradient, with a slightly bluer region on one side of the galaxy. This bluer region may be indicative of younger stars or increased star formation activity, though it should be noted this region is still relatively smooth. The color and morphology suggest that the galaxy could be an early-type spiral galaxy or possibly an elliptical galaxy that still exhibits some star formation. The relatively compact size implies that it is likely to be a galaxy at a moderate cosmological distance.
