The galaxy appears to be an elliptical galaxy, characterized by a smooth, diffuse light profile with no apparent spiral arms or prominent disk structure. It exhibits a high degree of central concentration, with a bright core that gradually fades into the outer regions. The overall shape is nearly round, with a slight deviation suggesting it is not perfectly spherical. There's no clear evidence of recent or ongoing merger activity, such as tidal tails or disrupted morphology. Color gradients within the galaxy are subtle, with the core potentially appearing slightly yellower, indicating an older stellar population compared to the outer regions. The galaxy's apparent size is relatively small, but this is consistent with its cosmological redshift, suggesting it is at a considerable distance. The low levels of current star formation further indicate that this is a relatively evolved system.
