The galaxy presents as a relatively smooth, elongated structure with a suggestion of two distinct nuclei or concentrations of light. The primary color appears to be a yellow-orange hue, indicative of an older stellar population. The overall shape is somewhat cigar-like, possibly hinting at a disk galaxy viewed at an angle or an elliptical galaxy. Some irregularities in the structure indicate a possible interaction or merger event, though major disturbances are not overtly apparent. There may be an indication of tidal tails or bridges between the two concentrations, suggestive of an ongoing merger.
