The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely spheroidal in shape with no prominent disk features discernible at this resolution. The galaxy's core exhibits a bright, concentrated luminosity, indicative of a high stellar density. A gradual decrease in luminosity is observed moving outward from the center, with a diffuse halo that extends to a significant radius. There is no strong evidence of tidal tails or significant asymmetries to suggest a recent major merger event. Subtle hints of minor disturbances could be present but further data would be needed to confirm. Overall, the galaxy appears to be a mature system, consistent with a relatively quiescent star formation history.
