The galaxy presents as a somewhat elliptical structure with a smooth, diffuse appearance. The light distribution suggests a concentration of stars towards the galactic center, exhibiting a yellowish-white hue, implying an older stellar population. There appears to be a gradual decrease in light intensity from the core outwards. The galaxy's overall shape is elongated, resembling a slightly flattened spheroid, with no distinct spiral arms or prominent features visible at this resolution. There is little evidence of dust lanes or significant star formation regions. There may be some subtle signs of minor asymmetry. The galaxy is generally compact. The redshift value indicates that this galaxy is at a considerable distance from our own.
