The galaxy presents as a single, well-defined object with a smooth, elliptical morphology. There is a notable concentration of light toward the center, suggesting a prominent galactic nucleus or bulge. The color appears to be predominantly yellow-orange, potentially indicating an older stellar population with a lower rate of star formation. No distinct spiral arms or dust lanes are discernible within the galaxy's structure. There does not appear to be any tidal distortions or evidence of recent merger activity. The overall symmetry and lack of significant substructure suggest a relaxed dynamical state. The object is relatively compact in size.
