The galaxy presents as a spiral type, exhibiting prominent spiral arm structures. These arms appear well-defined and extend significantly from the central bulge, indicating a grand design spiral pattern. The bulge component appears moderate in size, with a noticeable central concentration of light that graduates outwards, changing from yellow to bluish hues in the arms. The overall color suggests ongoing star formation activity, particularly within the spiral arms where the blue color is more pronounced. There is a weak bar-like structure present in the central region. The disk appears to be viewed at a moderate inclination angle. The galaxy appears to be interacting or merging with nearby smaller galaxy. The tidal interaction is causing gravitational distortion.