The galaxy appears as a system of two interacting galaxies, distinguished by their morphology and relative positions.

The larger, primary galaxy presents an elliptical shape, elongated along one axis. The light distribution suggests a relatively smooth profile, possibly indicating an older stellar population with minimal current star formation. The color is predominantly reddish-yellow, consistent with evolved stars.

The smaller, secondary galaxy is more compact and appears nearly spherical. This galaxy exhibits a more intense yellowish hue, hinting at a potentially younger stellar population or enhanced recent star formation activity compared to the primary galaxy.

The spatial proximity of these two galaxies, coupled with the observed asymmetry in the light distribution of the primary galaxy, implies gravitational interaction. There might be tidal disturbances or a merging process underway, altering the morphology of both galaxies. The system is located at a considerable distance, indicated by a redshift measurement of approximately 0.21, suggesting that we observe the galaxy as it was billions of years ago.

Overall, the observed system is likely a pair of interacting galaxies with differing morphologies and stellar populations, potentially undergoing a merger. Further spectroscopic analysis would be necessary to confirm the nature of the stellar populations and the dynamics of the interaction.
