The galaxy presents a primarily smooth morphology, exhibiting a fairly round appearance. There is a central concentration of light that appears golden in color. Based on the color distribution across the galaxy, the object appears relatively old, and mostly consists of older stellar populations. The absence of defined spiral arms or a clear disk structure supports this assessment. There appear to be some mild disturbances in the light profile suggesting a possible interaction or merger in the past. Overall, it presents as a fairly massive galaxy at a considerable distance.