The galaxy appears to be undergoing a significant interaction or merging event. Its morphology is highly disturbed. A bright, somewhat compact central region is observed. Emanating from this core are diffuse, tidal-like features, with a distinct plume or tail extending outward. There is no clearly defined spiral structure or elliptical shape. Patches of bluer coloration are present, suggesting regions of recent star formation. The overall color is yellowish-white, but the bluish regions could indicate an ongoing active star formation rate. The object looks asymmetric, likely due to gravitational disruptions from the interaction. This disturbance has caused a mass and star formation rate consistent with values from similar galaxies.
