The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a noticeable color gradient, with a bright, yellowish-white core that suggests an older stellar population. The outer regions appear bluer, possibly indicating the presence of younger, hotter stars, although this is less pronounced. The overall shape is somewhat elongated. There is no clear evidence of spiral arms or significant dust lanes visible in this image. There may be a slight distortion in its overall symmetry but overall it seems to be in a stable structure and not interacting with another galaxy. 
