The galaxy appears as an elliptical or lenticular type. Its morphology is characterized by a smooth, featureless profile. The light distribution suggests a centrally concentrated bulge, with luminosity decreasing outwards. The galaxy's color is relatively uniform, appearing yellowish-orange. This suggests a stellar population dominated by older, redder stars, with limited ongoing star formation. No prominent spiral arms or dust lanes are discernible. The galaxy's overall structure suggests it is a relatively evolved system, possibly nearing the red sequence. There is no evidence of any significant tidal disturbances or ongoing mergers.
