This galaxy appears to be a spiral galaxy, viewed at an oblique angle. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population. There is evidence of a disk component, with hints of spiral arm structure. The arms have a bluer color, indicative of younger stars and ongoing star formation, but they are not sharply defined, appearing somewhat diffuse. There may be some faint dust lanes visible, particularly along the edges of the disk. Overall, the galaxy's morphology suggests it is undergoing active star formation with an estimated stellar mass range of 10^9 to 10^10 solar masses. There is no clear visual indication of any major merger event, although minor disturbances within the galaxy cannot be ruled out.
