The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, featureless morphology, lacking any discernible spiral arms or bar. The central region appears slightly brighter, suggesting a concentration of stars or a possible bulge. The galaxy displays a color gradient, transitioning from bluer hues at one end to redder tones at the other. This may indicate variations in stellar populations or dust content across the galactic disk. There is no evidence of any significant tidal disturbances or ongoing mergers, suggesting a relatively isolated and quiescent system. The galaxy's light is significantly redshifted indicating a substantial distance. This galaxy's estimated size suggests it is comparable to smaller galaxies in the local universe. Considering it has a non-negligible star formation rate and a substantial mass, it is likely a spiral galaxy viewed edge-on.
