The galaxy appears as a largely smooth, elliptical-shaped object. Its color profile shows a concentration of light in the yellow-red part of the spectrum, suggesting an older stellar population is dominant. No distinct spiral arm structures are visible, and the light distribution is concentrated centrally, indicating a possible bulge. The galaxy displays high degree of roundness, exhibiting minimal asymmetry. No strong evidence of ongoing major or minor mergers are observed. The small effective radius, in conjunction with the color profile, suggests a higher concentration of evolved stars near the galactic center. There appears to be minimal evidence of recent star formation, but possibly not completely quiescent based on the color. Overall, the object is likely an elliptical galaxy at a redshift indicative of significant distance.
