The galaxy presents as an elliptical morphology, with a high degree of central concentration. The core appears bright and yellowish-white, suggesting an older stellar population dominating the nuclear region. The outer regions exhibit a gradual decline in luminosity, fading into the background sky. There is a slight flattening, it does not appear perfectly spherical. Faint blue colors are present in the disk, suggesting the presence of younger stars and some ongoing star formation. The galaxy exhibits a smooth overall texture. There is no apparent tidal debris or strong morphological distortions indicative of recent major merger activity, though some minor disturbances cannot be ruled out.
