The galaxy appears as a smooth, elliptical-like object with a high degree of central concentration. It exhibits a moderately elongated shape, resembling that of an intermediate elliptical galaxy. The light distribution suggests a relatively featureless structure, with no discernible spiral arms or prominent dust lanes visible in this imaging. The galaxy presents a color gradient, trending towards bluer hues in the outer regions and redder tones towards the core. This could possibly indicate older stellar populations concentrated within the galactic center and relatively younger stellar populations in the outskirts. No strong evidence of active star formation regions are seen. The overall morphology suggests that this galaxy is likely a relatively quiescent system. 
