The galaxy appears to be a merging system consisting of two distinct components. The primary galaxy exhibits a smooth, elliptical morphology, with a concentrated central bulge. Its color is generally yellow-white, indicative of an older stellar population and lower levels of on-going star formation. The secondary galaxy is more compact and displays a bluer hue, suggesting a younger, hotter stellar population and possibly higher star formation rates. The system overall shows evidence of interaction, with some possible tidal distortion. A clear merging signature can be noted.
