The galaxy exhibits a complex morphology, appearing neither entirely smooth nor purely disk-like. The central region displays a higher concentration of light, suggesting a bulge component. Faint features are visible, indicating possible spiral arm structures or tidal tails. The object shows characteristics of a possible ongoing or recent interaction with another galaxy; disturbances seem present. The overall color appears moderately red, potentially indicating an older stellar population or significant dust extinction within the galaxy. The estimated size suggests it is not particularly large, but the irregularities in its shape indicate it might be an actively evolving system.
