The galaxy presents as a smooth, rounded structure with a concentrated central bulge. The color gradient suggests a relatively old stellar population, transitioning from yellow in the core to a redder hue towards the outer regions. There is likely ongoing star formation activity as evidenced by bluer regions, but this is not the dominant process. The galaxy appears to be undergoing some interaction or disturbance based on its shape, possibly a minor disturbance, or a merger event. This is possibly influencing its morphology and contributing to the presence of disturbed features.
