The galaxy presents a roughly elliptical morphology, appearing as a diffuse spheroid of light. It exhibits a relatively smooth structure with no obvious spiral arms or a prominent central bar. The light distribution is concentrated towards the center, suggesting a dense stellar population in the galactic core. While the overall color is a neutral hue, some subtle variations are visible, potentially indicating regions of differing stellar populations or dust content. There appears to be some kind of merging or disturbance occurring to this galaxy.
