The galaxy presents a morphology suggestive of an ongoing or recent merger event. Two distinct luminosity concentrations are visible within the galaxy's overall structure. The northern concentration appears more diffuse with a yellowish hue, indicative of an older stellar population. The southern concentration is more compact and exhibits a greenish tint, which may indicate ongoing star formation. A faint tidal tail appears to be present. The overall color index indicates a relatively mature galaxy with moderate star formation.
