The galaxy appears as a lenticular or possibly an elliptical type, characterized by a smooth, diffuse light distribution. The main body of the galaxy shows a concentration of light toward the center that gradually diminishes outward. It has a prominent bulge component. The disk component appears relatively uniform, showing little evidence of spiral arm structure or distinct dust lanes, suggesting a later-type system that has either consumed or lost most of its gas and dust, or that the disk is viewed nearly edge-on, obscuring any spiral structure. The shape of the galaxy is elongated. The object is colored light orange-yellow. There's no clear evidence of active star formation regions. The overall morphology suggests a relatively evolved system with a dominant older stellar population. There do not appear to be signs of any major ongoing merger activity or tidal disturbances in this image.
