The galaxy presents as a relatively smooth and elliptical-like structure with a central concentration of light. The core region exhibits a yellowish hue, which gradually transitions to a bluish-white color in the outer regions. There is a subtle suggestion of a disk component, although the overall form lacks well-defined spiral arms or distinct features. Indications of some minor disturbances in the morphology are visible. A small fraction of the light might be attributed to an artifact. The galaxy does not appear to be undergoing a major merger, but some tidal disruption or interaction cannot be entirely ruled out. The radial color gradient suggests possible ongoing or recent star formation activity, particularly in the outer regions. Overall, the galaxy appears to be a system in a transitional state, possibly evolving from a more actively star-forming phase toward a more quiescent state.
