The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. The color profile indicates a central concentration of older stellar populations, exhibiting a yellowish-orange hue. Towards one end, a subtle shift towards bluer colors implies the presence of younger stars or regions of ongoing star formation, though it is not pronounced. The overall symmetry and lack of apparent tidal features suggest that the galaxy is relatively undisturbed, with no major recent merger events. A slight disturbance is noticeable in the blueish region, perhaps from a minor gravitational interaction or internal dynamics. The galaxy exhibits a moderate redshift, placing it at a significant cosmological distance. The shape is highly elongated and cigar shaped.
