The galaxy appears to be undergoing a significant merger event. The morphology is highly disturbed, showing no clear spiral arm structure or central bulge in the traditional sense. Instead, the light distribution is irregular and asymmetric. Two distinct, bright clumps of light are visible, suggestive of the merging cores of the progenitor galaxies. These cores appear connected by fainter material. The overall shape is elongated, with a degree of tidal distortion evident in the extended, diffuse outer regions. There's a general yellow/orange hue to the galaxy, possibly indicating an older stellar population. The relatively smooth appearance of the light suggests it is a red and dead galaxy. The colour may also arise from dust obscuration associated with the merger, although the resolution is insufficient to confirm this.
