The galaxy presents as a relatively elongated, cigar-shaped structure. It exhibits a smooth, featureless morphology, lacking apparent spiral arms or prominent dust lanes. There is a slight suggestion of a brighter central region, possibly indicative of a galactic bulge. Overall, the galaxy appears to be relatively isolated with no obvious signs of recent major merger activity or tidal disturbances, though some minor disturbance cannot be ruled out. The color profile suggests a population of older stars with a relatively low ongoing star formation rate. Given its redshift, the galaxy is situated at a considerable distance.
