The galaxy appears as a relatively small and faint object. It exhibits a predominantly red hue, suggesting an older stellar population. Its morphology seems largely amorphous, with a possible hint of a disk-like structure. Visual inspection hints at some disturbed structure, but more investigation would be needed to say whether it has undergone a recent merging event. However, this disturbance appears to be relatively minor in scope. The overall smoothness suggests it may be an elliptical galaxy or potentially a spiral galaxy, with little star formation.
