The galaxy presents as a centrally concentrated, smooth elliptical type. The core exhibits a bright, yellowish-white luminosity, suggesting a high density of older stellar populations. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness, fading into a diffuse halo. The halo appears relatively symmetrical and lacks any prominent spiral arm structures or distinct features, indicating a smooth distribution of stars. There is minimal evidence of dust lanes or active star formation regions within the galaxy, consistent with an older, more evolved system. The overall morphology suggests a dynamically relaxed galaxy, possibly formed through mergers in its past.
