The galaxy appears to be a relatively smooth, elliptical structure. It is characterized by a centrally concentrated bulge exhibiting a yellowish hue, suggesting an older stellar population. The overall light distribution is fairly even, with no distinct spiral arms or prominent dust lanes visible. The object shows a high degree of central concentration and a generally spheroidal morphology. There may be subtle disturbances present, but the galaxy appears to be mostly undisturbed. Its color suggests it has a low rate of star formation.
