This galaxy exhibits a clear disk-like morphology, viewed almost perfectly edge-on from our perspective. The central region presents a concentrated luminosity, suggesting a prominent bulge. The light profile of this bulge appears to be well-rounded. Dust lanes are not clearly delineated in this image, although there is a slight color variation moving from the center towards the edge of the disk. Given its redshift, the galaxy is likely a relatively massive system with a low rate of star formation. The galaxy appears relatively isolated, showing no strong signs of recent or ongoing merger activity. A faint object is visible on the left side of the disk, possibly a satellite galaxy or a tidal feature.
