The galaxy presents as a largely featureless, smooth object, with an elliptical morphology. The light is concentrated towards the center, and the galaxy appears to be highly symmetric with no prominent dust lanes or spiral arms. There is some slight suggestion of a disk-like structure at the center, but any features within this area are not defined. Its overall shape is neither perfectly circular nor highly elongated, existing somewhere in between. There is a potential minor disturbance visible in the galaxy, however it does not indicate any major ongoing merger events. The galaxy exhibits a subtle color gradient, appearing slightly bluer in the central region and redder in the outer regions. This color variation potentially reflects differences in stellar populations, with younger, bluer stars more concentrated towards the center and older, redder stars dominating the outer parts of the galaxy. The faintness and small size of the object suggests that it is at a considerable distance.
