The galaxy presents as an elongated structure, strongly suggesting an elliptical morphology. It exhibits a smooth light distribution across its body. The central region appears more concentrated and displays a reddish-orange hue, potentially indicating an older stellar population or significant dust obscuration. Moving outward from the core, the color gradually shifts toward a greenish tint, possibly signifying the presence of younger, bluer stars. The shape is distinctly cigar-like, with a high axial ratio, suggesting a possible classification as an E6 or E7 elliptical galaxy. There is no prominent sign of a spiral arm structure, and no presence of any major ongoing merger event.
