This galaxy exhibits a dominant, smooth central bulge that appears slightly elongated, transitioning to a more diffuse outer region. A discernible, though somewhat faint, disk-like structure is suspected, but the smoothness of the overall light distribution suggests a lack of prominent spiral arms. There is evidence of potential tidal disturbance to the left, and a subtle extension or plume originating from one side of the galaxy is visible, hinting at a possible interaction or merger event. The color gradient suggests the core of this galaxy is evolved, with the outer regions still forming stars.
