The object is a galaxy at a redshift of approximately 0.23. Morphologically, it appears to be a relatively smooth system, potentially an elliptical or S0 galaxy, exhibiting a high degree of central concentration. It is generally round in shape. There is no visually apparent indication of spiral arms or a distinct disk structure, nor any presence of major tidal disturbances or ongoing merger activity. The galaxy appears relatively isolated within its immediate environment. Its color indices suggest a population of older stars, consistent with a lower specific star formation rate. Overall, it looks like a fairly massive system.
