The galaxy presents a generally smooth, elliptical morphology, with a concentrated central bulge that exhibits a bright yellowish-white hue. This is potentially indicative of an older stellar population dominating the core. The galaxy's overall color profile suggests a relatively quiescent star formation rate, although there may be some ongoing activity as evidenced by some regions that appear slightly bluer. There are some faint, diffuse features extending outwards, but these lack clear definition. Overall, the galaxy shows a high degree of symmetry and lacks any obvious signs of significant tidal disturbance or major merger events. 
