The galaxy presents a flattened, disk-like morphology, observed at an inclined angle. A central bulge region is present, exhibiting a yellowish-white hue, indicative of an older stellar population. The disk component displays a bluer color, suggesting the presence of younger stars and ongoing star formation. The disk is relatively smooth in appearance, with little evidence of distinct spiral arm structures. Some minor disturbances or asymmetries can be observed within the disk. The overall color profile suggests moderate star formation activity and a substantial stellar mass.
