The galaxy presents as a somewhat flattened spheroid, with a smooth, diffuse light distribution that gradually decreases in intensity from its center outwards. The core region exhibits a brighter, more concentrated luminosity, suggesting a possible central bulge. The overall color appears to be slightly redder, indicating an older stellar population, possibly dominated by evolved stars. No distinct spiral arms or prominent dust lanes are apparent in the visible light image. The lack of well-defined features points towards a classification as an elliptical or lenticular galaxy, residing at a distance inferred from its redshift. The axial ratio indicates a moderate degree of ellipticity, deviating from a perfectly circular morphology. The galaxy shows no visible signs of recent merger activity or significant tidal disturbances, indicating a relatively quiescent evolutionary history.
