The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical morphology with no readily discernible spiral arms or disk-like structure. It has a relatively round shape, with a slight deviation towards an intermediate shape. The galaxy presents a central concentration of light, indicating a prominent galactic nucleus, surrounded by a more diffuse halo. There is a subtle color gradient, with the central regions appearing slightly redder compared to the outer regions, which are subtly bluer. This might indicate a population of older stars concentrated in the core, with younger stars inhabiting the galaxy's outer regions. No signs of major disturbances, such as tidal tails or interacting companions, are apparent, although there may be subtle signs of minor disturbances. These characteristics are indicative of a quiescent galaxy with a moderate star formation rate and a substantial stellar mass.
