The galaxy appears to be an elliptical system at a moderate redshift, with a generally smooth morphology. It presents a centrally concentrated bulge that diminishes in intensity outwards, suggesting a lack of significant spiral arm structures. The central region has a yellow-ish/orange-ish hue, potentially indicating a population of older stars. A slight amount of bluer light is detectable surrounding the core, implying some ongoing, though likely minimal, star formation activity. The galaxy's overall shape tends towards elliptical rather than a highly flattened disk. There are no prominent tidal tails or obvious signs of recent major merger events, although subtle asymmetric features might suggest minor disturbances or interactions.
