The galaxy presents a morphology suggesting an intermediate classification between elliptical and spiral. Its central region exhibits a concentrated, bright bulge with a yellowish hue. The overall shape is somewhat elongated rather than perfectly spherical. Fainter, disk-like features surround the core. There is evidence of slight asymmetry within the galaxy's structure. These disturbances might be indicative of a minor gravitational interaction or an internal dynamic process. The outer regions show hints of bluer star-forming regions. While some regions appear smoother, other parts of the galaxy exhibit subtle variations in brightness. These inconsistencies might suggest the presence of dust lanes or active star formation within the disk. Overall, the galaxy is not perfectly smooth; there are some areas with a more clumpy or diffuse appearance. The galaxy's light distribution is predominantly concentrated towards its core with a gradual decline in intensity towards its outer edges.
