The observed galaxy exhibits a morphology indicative of a merging system or a galaxy undergoing significant interaction. Two distinct luminous cores are apparent, suggesting the presence of two separate galactic nuclei in close proximity. The overall shape deviates significantly from a standard elliptical or spiral form; the structure is highly irregular and distorted, with diffuse stellar material extending outwards from the central regions. The color profile appears relatively uniform across the galaxy with a yellowish hue, suggesting an older stellar population dominating the overall light output and a low specific star formation rate. There is not much evidence of recent or ongoing star formation from the image alone. Evidence of possible tidal tails or bridges is uncertain due to the image resolution. The system appears to be in the advanced stages of merging based on the significant disruption of its original morphology.
