This galaxy appears to be a relatively smooth, elliptical system with a bright, concentrated central bulge. The galaxy exhibits a generally round morphology, with a very slight elongation. There is a noticeable color gradient, with the central region displaying a yellowish-white hue, suggesting an older stellar population. Moving outwards from the center, a subtle blueish tint can be observed, potentially indicative of a younger, though still relatively quiescent, stellar population or a low level of ongoing star formation in the outer regions. No distinct spiral arm structure or prominent dust lanes are discernible. The overall appearance is consistent with a galaxy that has largely completed its major mergers and is in a relatively evolved state. There's no strong indication of any recent or ongoing major merger activity, although there are a few slightly asymmetrical features, suggesting that minor disturbances or interactions may have occurred in the past.
