The galaxy presents as a centrally concentrated object, exhibiting a smooth morphology. The primary body of the galaxy is somewhat rounded in appearance. A noticeable color gradient exists, transitioning from a yellow-white core region to more red-shifted hues in the outer regions, suggesting potential variations in stellar populations or dust content across the galaxy. There seems to be a minor disturbance or possible merging event occuring, with a fainter portion appearing to be in close proximity with this galaxy.
