The object presents as a galaxy, observed at a redshift of approximately 0.1925. It appears relatively smooth and featureless, with a high degree of radial symmetry. The galaxy exhibits an elliptical morphology, showing a round shape with an apparently homogenous distribution of light, with a very high fraction of the light coming from a central bulge. Color gradients suggest a population of older stars, with a dominant population of cooler, redder stars in the galaxy's core. There is little evidence of ongoing or recent major star formation. No spiral arms or bar structures are apparent, nor is there a signs of current or recent mergers. The galaxy appears relatively isolated with no obvious tidal features.