The galaxy presents as an elongated, cigar-shaped structure, with a redshift indicating a significant distance. The light distribution suggests a central bulge with relatively smooth luminosity, surrounded by a fainter, more diffuse disk. The color gradients indicate a population of older stars dominating the bulge, while the disk shows bluer hues indicative of recent star formation. There is little evidence of strong spiral arm structure or prominent dust lanes in this image. Minor disturbances seem to be present, with a slight asymmetry in the disk that could indicate a past or ongoing interaction with a smaller galaxy. Overall, it appears to be an intermediately massive galaxy with moderate star formation activity.
