The galaxy presents an elliptical morphology, appearing cigar-shaped with a major axis notably longer than its minor axis. The light distribution exhibits a smooth profile, lacking discernible spiral arms or distinct clumps. The central region appears brighter and more concentrated, suggesting a prominent galactic nucleus. The galaxy exhibits a yellowish hue, possibly indicative of an older stellar population and lower levels of ongoing star formation. There is no visible evidence of tidal features or other signs of recent or ongoing mergers or interactions. Overall, the galaxy appears to be a relatively isolated elliptical galaxy at a moderate redshift.
