The galaxy appears to be a relatively smooth, elliptical-like object with a concentrated central bulge. It exhibits a generally rounded morphology with minimal discernible disk features. The color gradient suggests an older stellar population, with a yellow/red hue concentrated toward the galactic center, potentially indicative of a higher density of evolved stars. There might be some bluer regions in the outer parts of the galaxy. There does not appear to be a strong signature of any ongoing major merger activity or significant morphological disturbance, although there might be some indication of a minor disturbance.
