The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellow hue, suggesting an older stellar population. The outer regions display a bluer color, hinting at the presence of some younger stars or ongoing star formation, albeit at a relatively low rate. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy appears relatively undisturbed, showing no major signs of ongoing or recent merger activity. It appears fairly round in shape, with only a slight deviation from perfect circularity. Overall, this galaxy appears to be a massive system with a mix of stellar populations and a relatively quiescent star formation history.
