The galaxy presents as a roughly elliptical, smooth structure with no discernible spiral arms or bar. It has a concentrated central bulge, appearing nearly circular from our viewing angle. Color gradients suggest a relatively older stellar population. The core appears yellow/orange, indicative of evolved stars. The overall light distribution is relatively even, fading gradually toward the edges. The galaxy may be interacting, evidenced by a diffuse tail to the right, however the image is not sharp enough to definitively state this. The object may be a somewhat massive galaxy with a moderate star formation rate.
