The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated central region. The light profile suggests a centrally dominant luminosity. The galaxy exhibits a somewhat elongated shape, but it does not show any strong spiral arm structures or distinct features associated with active star formation. The color indices seem consistent with an older stellar population, indicating that star formation is currently low. There are no obvious signs of tidal disturbances or ongoing merging activity visible in the image.
