The galaxy presents as a somewhat elliptical, relatively smooth object with a central concentration of light. There is a distinct color gradient from the center outwards. The core appears to be a yellowish-orange hue, suggesting an older stellar population or significant dust obscuration. Surrounding the core is a fainter, slightly greenish halo. This suggests the presence of some younger, bluer stars, or ongoing star formation, however, star formation is low. The galaxy does not exhibit any prominent spiral arm structures, bars, or tidal features, indicating it is likely not undergoing any major interactions or mergers. Overall, the galaxy is of moderate size and luminosity at its redshift. Its morphology suggests it is either an elliptical galaxy, or a late-type spiral with a dominant bulge component and poorly defined spiral arms.
