The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. It appears generally rounded in shape, with a slight deviation from perfect circularity. There are hints of a disk structure, though faint. There is no visual evidence of any ongoing major mergers or significant tidal disturbances within this galaxy. There are a few faint hints of an outer structure. The color profile indicates an older stellar population. The overall appearance suggests a galaxy that is actively forming stars.