The galaxy appears to be an interacting system, possibly in the early stages of a merger. One galaxy has a smooth, elliptical morphology with a concentrated nucleus, displaying a yellowish hue indicative of an older stellar population. The other galaxy is more compact and exhibits a greenish tint, potentially indicating ongoing star formation. The system shows signs of tidal disturbance, with a slight elongation suggestive of gravitational interaction. The overall color distribution and morphology imply that the system is actively evolving.
