The galaxy presents a generally elliptical morphology, appearing somewhat rounded but leaning towards an intermediate shape. It exhibits a smooth, albeit slightly disturbed structure; some faint features are visible, indicative of a disk-like component or past interaction. The light distribution suggests a central bulge, with color variations indicating areas of differing stellar populations and dust content. Overall the galaxy appears to be experiencing ongoing star formation, judging by its colors. There might be evidence of minor disturbances suggesting a possible interaction or past merger event.