The galaxy exhibits an elongated, cigar-like morphology. It displays a relatively smooth light distribution, with a brighter, more concentrated central region suggestive of a bulge. One end of the galaxy shows bluer colors, potentially indicating a region of ongoing star formation, while the remaining region presents a redder hue. The overall structure hints at possible past or ongoing minor disturbances, although a complete merger is not immediately apparent. The galaxy appears to be undergoing some form of interaction or internal restructuring.
