The galaxy presents a relatively smooth and concentrated appearance. It appears to be an elliptical galaxy with a round morphology, showing no distinct spiral arm structures or prominent features indicative of ongoing major mergers. The galaxy exhibits a notable central bulge that gradually fades into the outer regions, exhibiting a diffuse halo. The color profile suggests the presence of a more aged stellar population. No clear dust lanes are visible. The overall appearance suggests a galaxy that has largely completed its major star formation phase and is relatively evolved.
