The galaxy exhibits a distinct spiral structure, with prominent, well-defined arms emanating from a central bulge. The arms display a bluish hue, indicative of ongoing star formation activity. There are areas of concentrated brightness within the spiral arms, likely regions of active star forming nebulae. The bulge appears relatively small, and it presents a whitish color, potentially suggesting an older stellar population. There are some signs of major disturbances and it is possible that the galaxy is undergoing a merging event with another galaxy. There also seem to be some indications of a bar feature running through the central region.
