This galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. The central region displays a bright, relatively smooth profile, appearing somewhat spheroidal. Extended features are evident, showing a distinct asymmetry. There are luminous knots present within the galaxy's structure that may indicate regions of heightened star formation. The overall color is indicative of an aging stellar population, but with regions showing bluer colors indicative of younger stars. There appears to be a tidal tail or stream of material extending from the main body of the galaxy, further supporting the merger scenario.
