The galaxy appears as a centrally concentrated object with a smooth overall morphology. It presents with a somewhat elliptical shape, exhibiting no discernible spiral arm structures or prominent features characteristic of a disk galaxy. The galaxy's color profile is predominantly reddish-yellow, suggesting an older stellar population or significant dust obscuration within the system. There appears to be evidence of a potential tidal interaction or ongoing merger event, based on a slightly disturbed morphology. There is some hint of possible disturbance in the system as well.
