This galaxy exhibits a morphology indicative of an ongoing or recent merger event. The primary structure appears generally smooth but disturbed, with an elongated shape. There is a possible tidal tail or bridge of material extending from the main body, suggesting gravitational interaction with another galaxy. The color profile suggests an older stellar population, with a yellow-red hue dominant, implying lower ongoing star formation. A secondary, smaller component is visible and appears distinct, indicating a potential merging partner. Some minor asymmetry can be observed. Overall, the galaxy appears to be in a late stage of merging, displaying significant signs of tidal interaction.
