The galaxy exhibits a generally elliptical morphology, though appearing somewhat disturbed. A fraction of its light is concentrated in a smoother component. The overall color is primarily redder, indicating an older stellar population. The galaxy displays potential signs of interaction or merging, with some asymmetry and possible tidal features extending from the main body. The estimated half-light radius suggests that the galaxy is relatively compact. It appears to have low star formation activity. There is also a hint of some bluer regions suggestive of ongoing, but low levels of star formation.
