The galaxy presents as a relatively smooth, centrally concentrated object. The morphology is primarily elliptical, exhibiting a high degree of radial symmetry. There is no obvious spiral structure, bar, or significant disk component visible in the image. The central region appears brighter and more compact than the outer regions, indicating a higher concentration of stars or possibly an active galactic nucleus. Color gradients are present; the core appears more yellowish-white, while the outer regions exhibit a bluer hue. This may indicate a population of older stars in the core and younger stars in the outer regions, suggesting ongoing, albeit possibly subdued, star formation. The overall structure indicates a galaxy that is well-evolved and likely of significant mass. There is no apparent interaction or merging activity occurring with other galaxies. The morphology is consistent with an early-type galaxy, likely an elliptical galaxy.
