The galaxy exhibits a somewhat elongated, cigar-like morphology. The color distribution suggests a bulge component that is yellower, possibly indicating an older stellar population. There are hints of a disk-like structure with bluer regions, potentially regions of ongoing star formation, though the image resolution limits a firm conclusion. Overall, the galaxy appears relatively smooth, with no clear signs of major disturbances or recent mergers, although subtle tidal features cannot be entirely ruled out. The galaxy has a red shift of roughly 0.235.
