The galaxy presents as a relatively smooth, elliptical-like structure. Its morphology appears largely undisturbed, with a high degree of central concentration. The light profile indicates a centrally bright core that gradually fades outwards. There is little evidence of distinct spiral arms or prominent dust lanes. The overall color suggests a stellar population that is older and redder on average. However, some bluer regions are present throughout the galaxy, indicating some ongoing star formation. There may be minor tidal features or asymmetries.
