The galaxy presents as a merging system, with two distinct luminous components. The larger component appears more diffuse with a warmer, yellower color, likely indicating an older stellar population or significant dust obscuration. The smaller component is more compact and exhibits a slightly bluer hue, suggesting ongoing star formation. There are hints of tidal features, particularly faint extensions and distortions around the main bodies, indicative of gravitational interaction. Overall, this appears to be a late-stage merger, potentially evolving towards a more relaxed elliptical morphology. There is a relatively high degree of smoothness in the overall light distribution.
