The galaxy appears to be a relatively compact object, with a smooth, elliptical morphology. Its light profile suggests a high degree of central concentration. The main body presents a yellowish hue, implying a significant population of older stars. There is a distinct blue region offset from the main body, possibly indicating a region of active star formation. This suggests that while the galaxy is primarily composed of older stars, there might be ongoing star formation. There are no obvious spiral arm structures present in the image. Overall, the galaxy gives the impression of a system transitioning from a more active, star-forming phase to a relatively quiescent state. There are hints of a possible interaction or tidal disturbance in the outer regions of the galaxy.
