This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated morphology. Its overall color is indicative of an older stellar population. The light is centrally concentrated, with a gradual decrease in surface brightness outward, lacking any distinct spiral arm structures or features indicative of active star formation. The shape is neither perfectly spherical nor highly elongated, appearing somewhere in between. There is no obvious evidence of tidal disturbances or ongoing mergers with other galaxies, which would suggest it is relatively undisturbed. The galaxy appears to have a substantial stellar mass, likely in the range of 10^10 solar masses.
