The galaxy presents as a relatively small, somewhat diffuse object. It appears to be undergoing a significant merger or disruptive event, exhibiting an irregular morphology. There is a bright central region, potentially indicating an active galactic nucleus or a high concentration of stars. Faint tidal features extend outward from the main body of the galaxy, suggesting gravitational interactions and recent or ongoing accretion. Based on the color indices, it is likely that star formation is still occurring, although perhaps at a low rate. The overall light profile indicates a relatively low mass object.
