The galaxy appears as an elliptical structure, exhibiting a smooth morphology with a concentrated central bulge. The color profile suggests a predominantly older stellar population, likely dominated by redder giants. The apparent smoothness indicates a lack of significant ongoing star formation. There is some asymmetry, or potential minor disturbance, in the distribution of light, which could be indicative of a past merger event or tidal interaction, though the overall structure remains largely undisturbed. Its size is consistent with a typical elliptical galaxy at its redshift. A slight elongation suggests that it is of intermediate shape.
