The galaxy presents an elliptical morphology, characterized by a smooth and rounded light distribution. The dominant color is a yellow-orange hue, suggesting an older stellar population with a lack of ongoing star formation. However, there appears to be a small, somewhat elongated blue region that may indicate some ongoing star formation.

A slight disturbance in the overall structure hints at a potential interaction or recent merger event. There is evidence of asymmetry or faint tidal features, such as possible distortions in the galaxy's outer regions, indicating an ongoing interaction or merger.

Overall, the galaxy presents a fairly relaxed and somewhat passive state, possibly transitioning from a star-forming disk galaxy to a quiescent elliptical galaxy.
