The galaxy presents an overall elliptical morphology, though there is some suggestion of a disk-like structure within the broader shape. The central region exhibits a high concentration of light, appearing bright and yellow in color. There is a surrounding envelope of fainter, bluer light that extends further out from the nucleus. This extended region appears relatively smooth, with only subtle variations in brightness. No distinct spiral arms or significant dust lanes are immediately apparent. The galaxy appears relatively isolated and unperturbed, lacking any obvious signs of recent mergers or tidal interactions. There is a slight asymmetry, indicating a potential distortion in its morphology. The object is moderately redshifted, suggesting a substantial distance and lookback time. The object's appearance is indicative of a relatively evolved system that has likely undergone significant internal processing and exhibits a low rate of star formation.
