The galaxy presents an overall elliptical morphology, with a smooth light distribution, and a high Sersic index. The core exhibits a bright, concentrated luminosity. The axial ratio indicates that the galaxy is moderately flattened. The color indices suggest the presence of an evolved stellar population, with a redder color in the central regions. There are no apparent spiral arm structures or significant dust lanes, indicating a relatively quiescent galaxy without recent major merger events.
