The galaxy presents as an elongated, somewhat disturbed system. It appears to be undergoing a possible merger event, indicated by the dual core structure. One core is more diffuse and elongated, with a bluer hue, potentially indicating ongoing star formation. The other core appears more concentrated and exhibits a warmer, redder color profile suggesting an older stellar population. There appears to be some tidal tail formation extending from the galaxy, indicating gravitational interaction. The overall morphology is complex, showing signs of significant disturbance.
