The galaxy presents as a single, cohesive structure exhibiting a generally smooth morphology. The galaxy appears to be in a relatively advanced stage of its evolution, with a noticeable lack of prominent spiral arms or distinct substructures typically associated with active star formation. There is an elliptical appearance with an elongation. The color gradient transitions from a central, yellowish hue to a more diffuse, greenish-blue periphery, indicative of a shift in stellar populations across the galactic radius. It may be undergoing or have recently undergone a merging event with another galaxy. There is a single bright core which is slightly off-center.
