The galaxy presents as an elongated structure, with a central, highly concentrated region exhibiting a primarily smooth texture. The morphology appears to be undergoing significant disturbance, as evidenced by a prominent tidal tail extending from the main body. This tail displays a reddish hue, suggestive of older stellar populations or dust obscuration. The galaxy is generally smooth in appearance, however, a secondary, less distinct feature extends from the opposite side of the main body, hinting at a more complex interaction or internal structure. Overall, the galaxy appears to be in a late stage merger.
