The galaxy appears to exhibit a complex morphology, potentially indicating an ongoing interaction or recent merger event. The system displays two distinct luminous components. One is an extended, diffuse structure with a relatively smooth appearance. The second component appears more compact and exhibits a bluer color profile, possibly indicative of younger stellar populations or active star formation regions. There appears to be a tidal tail or bridge-like feature extending from the second component, suggesting a gravitational interaction. The overall color gradient suggests a transition from bluer, actively star-forming regions to redder, older stellar populations within the galaxy. A small asymmetry is apparent in the overall structure.
