The galaxy appears to be undergoing a merger, with two distinct components visible. The larger component shows a generally smooth morphology, with a bright, concentrated core. There is a subtle color gradient across this primary galaxy, with a redder hue towards one edge, possibly indicating an older stellar population or dust obscuration in that region. The second component is bluer in color, suggesting more active star formation. It exhibits a less defined structure than the primary component. The two components are clearly interacting, as evidenced by the visual distortion of each. There appears to be faint tidal debris or connecting structures between the two components, indicating that the interaction is ongoing. The overall structure does not resemble a well-defined spiral or elliptical galaxy in its relaxed state, thus exhibiting signs of a recent disruptive event like the galaxy merger. 
