The galaxy presents a complex morphological structure, potentially indicative of an ongoing or recent interaction or merger event. The primary galaxy exhibits a relatively smooth, though not perfectly elliptical, light distribution with a concentrated central bulge. The overall color appears to be redder, suggesting an older stellar population and potentially lower ongoing star formation activity. A fainter secondary component is observed in proximity to the primary galaxy. This component has a more elongated morphology, possibly a disk, oriented at an angle relative to the major axis of the primary galaxy. The system exhibits subtle tidal features or distortions in the outer regions, possibly indicative of gravitational interactions. The estimated physical size suggests that the galaxy is relatively large. Overall, the system appears to be a massive galaxy with signs of recent or ongoing interaction, possibly influencing the morphology and star formation history.
