This galaxy presents a smooth, elongated morphology, appearing cigar-shaped. A likely spiral galaxy seen edge-on. The central bulge exhibits a brighter, concentrated luminosity gradient, fading outwards along the galactic disk. A hint of blue light emanating from the disk suggests the presence of younger, hotter stars within. The dust lane is difficult to discern, possibly due to the angle, but there is a hint of obscured light. The overall color is moderately blue-white. There may be minor disturbances due to a potential past merger event. The galaxy's general structure suggests it is relatively quiescent, not exhibiting strong signs of on-going, major star formation.
