This galaxy presents a generally elliptical morphology. The light distribution indicates a high degree of central concentration, appearing smooth with a largely featureless profile. The core exhibits a yellowish-white hue, suggesting an older stellar population with relatively low ongoing star formation, though a subtle presence of bluer light in the outer regions hints at some degree of recent or continuing star formation activity. The galaxy shows a subtle degree of flattening; however, there are no indications of prominent spiral arms or a well-defined disk structure. The color gradients appear smooth and gradual, with no signs of major disturbances such as tidal tails or morphological peculiarities indicative of recent major merger events. Overall, it exhibits characteristics consistent with a relatively evolved system.
