The galaxy presents a largely smooth morphology. The light profile suggests a central bulge that dominates the overall luminosity. The shape is approximately round. There's little indication of spiral arm structure or a distinct disk component, suggesting the galaxy is most likely an elliptical or lenticular type. The color appears relatively uniform and redder in comparison to typical spiral galaxies, indicating an older stellar population and a low rate of current star formation. There's no obvious sign of tidal disturbances or ongoing merger activity. Overall, the galaxy appears to be a relatively quiescent, evolved system.
