The galaxy appears as a centrally concentrated object with a smooth, relatively featureless morphology. There is a distinct bulge component that dominates the core of the galaxy, exhibiting a yellowish-white hue. The outer regions of the galaxy transition to a fainter, bluer color, suggesting the presence of a disk component.

The galaxy appears relatively isolated with no obvious signs of a major ongoing merger or significant tidal disturbances. There are no prominent spiral arms visible, and the overall structure indicates it is likely either an elliptical galaxy or a lenticular galaxy seen face-on, with a preference toward the former due to the smoothness. The galaxy is likely a massive system, with modest star formation occurring.
