The galaxy presents as an elliptical structure, elongated along its major axis. The core exhibits a concentrated, bright luminosity, suggesting a high density of stars or potentially an active galactic nucleus. The light profile appears smooth and diffuse, lacking any distinct spiral arm features or prominent dust lanes. The color is generally yellowish-orange, indicative of an older stellar population with relatively lower levels of ongoing star formation. The overall morphology suggests an evolved system, likely a lenticular or elliptical galaxy observed at a redshift that places it at a considerable distance. There might be a minor tidal disturbance, but the galaxy does not seem to be undergoing a major merger.
