The galaxy presents as an elliptical structure with a moderate redshift. It exhibits a relatively smooth morphology, appearing mostly featureless with no strong spiral arms or a prominent central bulge. The light distribution is somewhat concentrated towards the center, suggesting a high degree of central stellar density. There is a slight elongation in its shape, deviating marginally from a perfect circle towards a more in-between shape. The color profile indicates a mix of stellar populations, with reddish hues indicating older stars and bluer regions possibly indicating younger star formation, though the galaxy appears to be dominated by older stars. There are no obvious signs of a major ongoing merger, however, there are signs of minor disturbances in the morphology, indicating potential past interaction with smaller galaxies or tidal effects from neighboring galaxies.
