The galaxy presents as a complex system, exhibiting evidence of an ongoing or recent merger event. The primary body of the galaxy displays a diffuse, somewhat irregular morphology with a high degree of central concentration, potentially indicating an older stellar population and significant bulge component. There is a prominent tidal feature extending from the central region, suggesting gravitational interaction with another galaxy. 

The color profile of the central region appears relatively red, whereas bluer light, potentially indicating younger stars are observed in the outer regions. The general shape is roughly elliptical, but the tidal feature disrupts any smooth profile. There are multiple luminous knots visible, which might indicate regions of high star formation activity.
