The galaxy presents as a relatively smooth, centrally concentrated system. It exhibits a somewhat elliptical morphology, not perfectly circular, nor distinctly elongated. There appears to be no strong spiral arm structure visible, nor a distinct bar feature. A hint of a disk-like structure might be present, though it isn't clearly defined. The color profile suggests a composition of older stellar populations. There appears to be little evidence of significant ongoing star formation. There is only a slight color variation throughout the galaxy, being more blue towards the center, indicating the possibility of slightly younger stars or perhaps more heavy metals. The galaxy's overall structure appears relatively undisturbed, without any strong signs of recent major merger events. There is a subtle asymmetry present.
