The galaxy appears to be a spiral type, exhibiting a relatively high degree of organized structure within its disk. The spiral arms are prominent and traceable, with a well-defined morphology, potentially displaying a grand design. There seems to be two dominant spiral arms. The arms appear loosely wound. The central bulge is noticeable, demonstrating a moderate contribution to the overall luminosity of the galaxy. The color gradients suggest active star formation regions along the spiral arms, with the presence of bluer components. Overall, the galaxy appears to be isolated with the possibility of tidal disturbances.
