The galaxy presents as a pair of interacting or merging objects. Each component exhibits a relatively smooth, rounded morphology, though subtle tidal features and distortions are possibly present. One of the components appears slightly more elongated or cigar-shaped than the other. The color distribution suggests an older stellar population, with a redder hue dominating. There is very little, if any, evidence of significant ongoing star formation or prominent spiral arm structure. The overall appearance is suggestive of a system undergoing a relatively late-stage merger.
