The galaxy presents a generally smooth morphology, appearing largely featureless. Its overall shape is elliptical, exhibiting high degree of circularity in its structure. The central region displays a bright, concentrated core that suggests a high stellar density. The galaxy's color profile appears to be trending towards the redder end of the spectrum, suggesting a predominantly older stellar population with relatively low ongoing star formation. There is very slight evidence of faint extensions, but these could just be an artifact. No strong signs of spiral arms or a prominent disk component can be distinguished. No major merger events appear to be in progress, although some minor asymmetries might suggest previous interactions or disturbances.