The galaxy presents as a distorted spiral, or possibly an elliptical galaxy with faint tidal features. The central bulge appears prominent and elliptical in shape, with a yellowish-white color suggesting an older stellar population. A fainter, diffuse component extends outward, with a slight curvature suggestive of a disrupted disk or tidal tail. The overall morphology indicates a galaxy that is not entirely relaxed. There is evidence of recent or ongoing gravitational interaction. The light profile is dominated by the bulge, but with extended, asymmetric features that deviate significantly from a smooth elliptical isophote. The galaxy exhibits a redshift within the range expected for galaxies at intermediate distances, indicating we are observing it at a considerable lookback time. The color gradients suggest possible variations in stellar populations or dust obscuration across the galaxy. Further spectroscopic analysis would be needed to confirm the nature of these features and to characterize the star formation history.
