The galaxy presents as a pair of closely interacting or merging galactic structures. The larger of the two components exhibits a predominantly smooth morphology, with a slightly elongated, cigar-like shape. Its central region appears brighter and exhibits a reddish-orange hue, potentially indicating an older stellar population or dust obscuration. The outer regions appear more diffuse and slightly bluer, suggestive of ongoing or recent star formation.

The smaller component is positioned adjacent to the larger galaxy. It appears more compact and rounder in shape, displaying a more uniform reddish-orange color. The proximity and color suggest tidal interactions. There is no strong evidence of a significant disk structure. Overall, the system is likely in a relatively late stage of interaction, potentially leading to a single, elliptical-like galaxy in the future.
