The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. Its light profile seems highly concentrated towards the center, with a gradual fall-off in intensity outwards. The galaxy exhibits a yellowish-white hue, suggesting a population dominated by older stars, given its color properties. There is no apparent spiral structure or distinct dust lanes visible in this image. The lack of blue coloration suggests that star formation activity may be low. There is no visual indication of any major ongoing merger events. The morphology appears generally regular, with a mostly round appearance. 
