The galaxy appears as a roughly circular, centrally concentrated object. It exhibits a smooth morphology. The galaxy displays a generally greenish hue, indicating a higher relative flux in shorter wavelengths such as g-band. A linear feature, appearing in the bluer wavelengths, intersects the galaxy near its center, possibly indicating a spiral arm viewed edge-on or an artifact. There is some subtle distortion of the galaxy's shape suggesting a possible interaction, but no distinct merging features are apparent. Minor disturbances are possible based on the slight asymmetries observed in the galaxy's light distribution, and the central concentration suggests it may be an elliptical galaxy or a spiral galaxy viewed from a particular angle.
