The galaxy exhibits a flattened, elliptical morphology with a relatively smooth light distribution. It appears to be a disk galaxy with an inclination towards our line of sight. The central region displays a brighter, more concentrated luminosity profile, suggestive of a bulge component. The outer regions fade gradually, indicating the presence of a stellar halo or a more diffuse disk. The galaxy presents a bluish-white hue, which is likely due to the presence of young, hot stars. There is a hint of internal structure, possibly faint spiral arms or dust lanes, however, the image resolution limits precise characterization. Overall, the galaxy appears to be relatively undisturbed and undergoing moderate star formation activity.
