The galaxy presents a disk-like morphology, with a noticeable bulge at its center. The overall color profile indicates a mature stellar population, particularly in the central bulge region, which appears yellowish-white, suggesting older, cooler stars dominate. There are subtle hints of bluer regions in the disk, potentially indicative of younger stars and ongoing star formation. The disk itself exhibits some irregularities and distortions, possibly due to interactions or internal dynamics. There is faint red areas on the edges of the galaxy, which could be areas with dust obscuring the light. The galaxy appears somewhat elongated, with the disk oriented at an angle relative to our line of sight.
