The galaxy presents as a relatively compact object with a smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, indicating a high density of stars in the central region. The color gradient suggests a population of older stars, potentially with ongoing low levels of star formation. There is a hint of a faint, disk-like structure extending outwards, though the resolution limits detailed analysis. No obvious signs of spiral arms or significant tidal disturbances are apparent, suggesting a relatively undisturbed evolutionary history. The overall appearance points towards an early-type galaxy, possibly undergoing a transition between a spiral and elliptical form.
