The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated light profile, with the highest luminosity emanating from the core. Moving outwards, the light gradually diminishes without distinct spiral arm structures or prominent star-forming regions. There are no obvious signs of a recent major merger or tidal disturbances affecting its overall morphology, though there may be a slight irregularity or minor disturbance on one side. The galaxy presents an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. The color suggests a population of older stars, with little evidence of ongoing, significant star formation. 
