The galaxy presents a generally smooth and rounded appearance, suggesting an elliptical or lenticular morphology. Its light profile appears centrally concentrated with a gradual decrease in intensity outwards. There is a subtle color gradient, shifting from bluer hues in the central region to slightly redder tones in the outskirts. The galaxy does not exhibit any prominent spiral arms or distinct features indicative of active star formation regions at this resolution. A slight asymmetry may be present but this would need further inspection with more detailed data. There is no clear evidence of ongoing merger activity or major tidal disturbances.
