The galaxy presents a generally smooth, elliptical morphology, displaying a notable concentration of light towards its central region. The core exhibits a yellowish-orange hue, suggesting a population of older stars. The outer regions transition to a slightly bluer color, potentially indicating some ongoing star formation, albeit at a modest rate. There is no immediately obvious evidence of significant disk structures or spiral arms. The overall shape is largely round. There are no prominent tidal features or major disturbances, suggesting it is likely not undergoing a major merger. Minor disturbances cannot be ruled out.
