The galaxy presents as a merging system, exhibiting significant gravitational disturbance. Two distinct galactic nuclei are visible, their cores appearing concentrated and luminous. The overall morphology is highly irregular, lacking defined spiral arms or a clear elliptical structure. A significant fraction of the system's light is concentrated in the central region between the two nuclei, suggestive of intense star formation or tidal interactions. Faint, diffuse extensions, potentially tidal tails, are suspected, although the resolution is insufficient for definitive confirmation. The color of the galaxy is predominantly yellow-orange, indicating a population of older stars and a relatively low ongoing star formation rate, although regions of blue suggest areas of more recent star formation.
