This galaxy exhibits a generally elliptical morphology, although it presents a slight disk-like appearance. The central region of the galaxy appears bright and concentrated with a yellowish color, suggesting a population of older stars. Moving outward from the center, the galaxy fades gradually into a bluish halo or disk, indicating a younger stellar population and potentially ongoing star formation in these regions. There is a moderate amount of dust obscuration, but overall, the galaxy's structure seems relatively smooth, with no apparent strong spiral arms or significant morphological disturbances. The ellipticity of the galaxy suggests it may be close to edge-on from our point of view, leading to the elongation observed.
