The galaxy exhibits a complex morphology, appearing to be in a state of interaction or merger. The central region displays a relatively smooth, concentrated light distribution with a yellow hue, possibly indicating an older stellar population. Extending outwards from the central region is a fainter, more diffuse blueish structure that appears elongated, with an overall cigar-like shape. The overall color suggests the presence of some ongoing star formation, even if diminished. The galaxy's general structure suggests a system that is undergoing significant gravitational disturbance.
