The galaxy presents as a relatively smooth, elongated structure, suggestive of an elliptical morphology. It exhibits a core region that is brighter and more concentrated. There may be a faint disk present, although it is not clearly visible. Overall, the structure is fairly regular, with some evidence of possible minor disturbances. The color distribution indicates a mix of stellar populations, with slightly bluer regions possibly representing areas of recent star formation, and redder regions likely dominated by older, more evolved stars. There is some evidence of merging events, although they appear to be relatively minor.
