The galaxy presents a somewhat amorphous structure, appearing largely smooth with a slightly elongated shape. There is a prominent central bulge that appears to be slightly off center. The color distribution suggests a population of older stars, possibly with a lack of significant on-going star formation within the central region. Fainter, diffuse extensions are observed, which may indicate tidal interactions or past mergers. Overall, the galaxy appears to be in a state of interaction or recent interaction based on its morphology and color distribution. The overall color profile suggests an intermediate redshift object.
