The galaxy presents as a moderately redshifted, luminous object with an elliptical morphology. It exhibits a smooth, centrally concentrated light profile, appearing generally featureless in this observation. The galaxy displays a distinct elongation, resembling a cigar shape. Its color profile suggests a relatively old stellar population, potentially indicating a lower specific star formation rate. There is no immediately obvious evidence of significant ongoing mergers or major disturbances in its structure. Faint disk features may be present. 
