The galaxy presents as a relatively compact, luminous object. Its morphology appears largely smooth and elliptical, lacking prominent spiral arms or a distinct disk structure. The color profile suggests a dominance of older stellar populations, trending towards redder wavelengths, which implies a lower rate of on-going star formation. There is no evidence of significant tidal disturbances or ongoing mergers based on the smoothness of its structure, however, there may be minor disturbances present. The overall shape is primarily in between round and elliptical, with no elongated features visible. The concentration of light is highest toward the center, gradually decreasing outwards, suggesting a centrally concentrated mass distribution. Given these characteristics, the galaxy is likely an elliptical galaxy at moderate redshift.
