The galaxy presents as an elliptical or lenticular morphology. The central region exhibits a concentrated, bright nucleus, decreasing in luminosity with radial distance. The overall color is primarily redder hues, suggesting a stellar population dominated by older, evolved stars. There is a slight blue tint in the outer edges. The galaxy appears relatively smooth, lacking prominent spiral arms or distinct features. There is no evidence of major tidal disturbances or ongoing mergers, though some faint asymmetry is present in the outer halo. Based on this, the object is likely a massive galaxy with a substantial stellar mass, a low specific star formation rate and a redshift of approximately 0.23.
