The galaxy presents as a disturbed system, possibly undergoing a merger or significant interaction with another galaxy. The central region displays a concentrated luminosity, with a relatively smooth, albeit somewhat irregular, morphology. Evident is an extended structure, potentially a tidal tail or distorted spiral arm, suggesting gravitational interaction. Patches of bluer light are visible, which may indicate areas of active star formation. The overall color index suggests a population of both older, redder stars and younger, bluer stars. There is no clear disk structure and no apparent spiral arms.
