The galaxy presents as a relatively smooth, elliptical-shaped structure, with a concentrated central bulge and a faint extended halo. The overall color of the galaxy appears to be yellowish-white, indicative of an older stellar population with fewer young, massive stars, and a moderate amount of dust extinction. There is no obvious spiral structure or distinct features such as prominent star-forming regions or dust lanes. The galaxy exhibits a high degree of central concentration, suggesting a relatively relaxed system. There is no obvious evidence of a major merger or strong tidal interactions.
