The galaxy presents as a somewhat elongated, elliptical structure. It exhibits a smooth, largely featureless morphology. The central region displays a high degree of luminosity, suggesting a concentrated stellar population or active galactic nucleus. The color profile shifts from a whiter core, transitioning to a slightly yellower hue towards the outer regions. No distinct spiral arms or bar structures are discernible. The galaxy appears relatively isolated, showing no obvious signs of major ongoing mergers or tidal disturbances, though subtle asymmetries could indicate minor interactions in the past. Its overall appearance aligns with that of a typical early-type galaxy, potentially an elliptical or lenticular system observed at a moderate redshift.
