The galaxy presents a generally smooth morphology with an apparent central bulge. There are hints of a distorted disk structure, possibly indicating a recent or ongoing interaction with another galaxy, or internal disturbances. The object is not perfectly circular but is somewhat elongated. There are some subtle irregular features present, suggesting some level of dynamical activity. There is a component with an apparent green hue to the galaxy and a second component with a redder hue that appear to be in the process of merging. 