The galaxy presents as a moderately bright object with a noticeable disk-like structure. There appears to be ongoing or recent merger activity, showing signs of tidal disturbances or interactions. A substantial fraction of the galaxy's light is distributed smoothly, though there are some indications of patchy structures within the disk. Overall, the light is fairly concentrated towards the center of the object. The galaxy is slightly elongated. It displays colors suggesting a mix of stellar populations, with the bluer components likely indicating ongoing star formation.
