The galaxy presents a generally smooth and rounded morphology. It appears to be an elliptical galaxy, with no discernible spiral arms or bar structure. The core exhibits a high surface brightness, with a central concentration of light. Moving outwards from the core, the light gradually diminishes. The galaxy has a slight blue tint in the surrounding halo which may indicate ongoing star formation. There is no strong evidence of tidal disturbances or recent merger activity. The light is evenly distributed with a generally symmetrical shape.