The galaxy presents as a mostly smooth, centralized light distribution. The object exhibits an elliptical morphology, though some asymmetry is noted. The central region demonstrates a high degree of luminosity, indicating a dense concentration of stars, or possibly an active galactic nucleus. Fainter light extends outwards, and the system appears to be undergoing no major mergers. There are hints of spiral arm structures, though they are not prominent and appear tightly wound. Overall, the galaxy presents as an evolved system with a substantial bulge component. The color of the galaxy is largely yellow, indicating older stars.
