The galaxy presents a generally smooth and concentrated morphology. It exhibits a centrally bright core with a significant radial decrease in surface brightness outwards. The overall color profile suggests a redder nucleus transitioning into slightly bluer outskirts. There are no prominent spiral arm structures or obvious dust lanes visible. The isophotes appear largely elliptical, with a moderate degree of ellipticity, being neither perfectly round nor highly elongated. There is little evidence of ongoing major merger activity or significant tidal disturbances. The galaxy appears relatively undisturbed, indicating a possible state of quiescence or a slow, steady rate of star formation.
