The galaxy appears to be a relatively small, faint object. Its morphology is difficult to classify definitively, but there is evidence suggesting the presence of some features or a disk-like structure. There is evidence of potential minor and major disturbances, though the galaxy appears largely unmerged and not experiencing significant interaction with any major galaxy. The color profile indicates a range of stellar populations, with a higher concentration of red stars. The image shows indications of a possible merger event, or signs of tidal disruption.