This galaxy appears to be a disk galaxy at intermediate redshift. It exhibits a relatively bright, compact core that transitions into a more diffuse, extended halo. The core shows a blue color, suggesting a significant population of young, hot stars, which is indicative of active star formation. 

There is evidence of structural disturbance within the galaxy, possibly resulting from a minor merger or interaction with another galaxy. This is suggested by the slightly irregular morphology and faint tidal features extending from the main body. The galaxy is moderately luminous, inferring a substantial stellar mass. The overall blue color indicates ongoing star formation occurring at a moderate rate, contributing to its luminosity.
