The galaxy presents as an elongated, cigar-shaped system, with a relatively smooth, featureless appearance across its main body. It exhibits a color gradient, transitioning from a yellowish-white central region to bluish hues at its outer edges. This may suggest ongoing or recent star formation in the outer regions, with the central area potentially dominated by older stellar populations. The high degree of elongation indicates that this may be a spiral galaxy that is seen nearly edge-on. No prominent dust lanes or spiral arms are visible, possibly due to the viewing angle or the galaxy's overall structure. No tidal distortions or signs of an ongoing merger are clearly visible within the image. The galaxy appears relatively isolated and undisturbed.
