The galaxy presents as a relatively compact object. The light profile appears smooth and centrally concentrated, exhibiting a morphology consistent with an elliptical galaxy. The color index indicates that it is relatively redder than a typical spiral galaxy, suggesting an older stellar population or significant dust extinction. There is little to no evidence of spiral arm structure or a prominent disk. The galaxy seems to be relatively undisturbed, showing no signs of ongoing major mergers or tidal interactions. The shape is somewhat elongated, but generally close to circular, but closer inspection suggests that the galaxy may be "In Between" circular and elongated. 
