The galaxy appears to be undergoing a significant merging event. Two distinct, luminous regions of the galaxy are visible, suggesting the remnants of two progenitor galaxies. There is a large, yellowish central region, surrounded by a diffuse, fainter halo. The morphology is disturbed, and there are no discernible spiral arms or a well-defined disk structure. The relatively smooth appearance and color profile suggests a population of older stars. There is also a very faint reddish region separated from the bulk of the galaxy.
