The galaxy appears to be a single, luminous object with a generally smooth morphology. It exhibits a slightly elongated, round shape, with no distinct spiral arms or bar structure visible. The central region is brighter and appears yellowish, suggesting an older stellar population. The outer regions of the galaxy fade gradually into the background, presenting a less intense, somewhat reddish hue. There is no evidence of significant dust lanes, tidal tails, or other major disturbances that would indicate ongoing merging activity. The galaxy appears relatively isolated and undisturbed. The redshift indicates that this galaxy is at a significant distance. The galaxy has a moderate size, consistent with a typical galaxy size for this redshift.
