The galaxy exhibits a morphology consistent with an ongoing or recent merger event. The primary body of the galaxy appears relatively smooth, with a somewhat elliptical profile. A secondary, distinct component is visible, suggesting a possible smaller galaxy interacting with the main structure. There is some indication of tidal features or disturbances, potentially signifying gravitational interaction. Overall color is yellowish-white, possibly indicating an older stellar population, but some redder regions are visible, potentially pointing to some ongoing star formation in certain areas.
