The galaxy presents as a centrally concentrated, elliptical-like structure, appearing largely smooth in texture with a high degree of central luminosity. There is an apparent lack of defined spiral arm structures, dust lanes, or other prominent features typically associated with disk galaxies. The dominant color is a yellow-orange hue, suggesting an older stellar population with lower rates of ongoing star formation. The galaxy appears relatively isolated, with no clear signs of major tidal interactions or ongoing mergers with other galaxies, though subtle asymmetric features may be indicative of minor disturbances. The overall morphology indicates a system with a likely significant mass, consistent with an evolved elliptical galaxy that is not highly active. The redder color and smooth appearance aligns with a galaxy where star formation has significantly decreased over time, leading to a dominance of older, redder stars.
