This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of luminosity, indicating a concentrated stellar population and/or active galactic nucleus. The core color is distinctly yellow-orange, suggesting an older stellar population, as younger, bluer stars have largely evolved off the main sequence. Progressing outward from the core, the luminosity decreases, and the color subtly shifts toward green hues in the outer edges, indicating a smaller presence of younger stars and ionized gases. The observed ellipticity is significant, meaning that the galaxy appears elongated, almost cigar-shaped. There are no prominent spiral arms or obvious signs of recent major merger activity; however, some minor asymmetries or subtle disturbances in the outer halo suggest possible previous interactions. Overall, this galaxy appears to be a massive, evolved system with signs of past activity but currently exhibiting relative quiescence in its star formation.
