The galaxy presents an irregular morphology, suggestive of an ongoing or recent interaction. Its overall color is yellowish to reddish, indicative of an older stellar population with a lower rate of star formation. The main body of the galaxy is elongated, with a brighter, more concentrated region near the center, likely representing the galactic nucleus. A distinct, smaller luminous component is observed to be in close proximity, which could be a satellite galaxy or a tidal feature resulting from a merger event. The image suggests a mass of 10^11 solar masses. There's evidence of disturbance, as evidenced by the irregular shape, potentially indicating an early stage merger.
